The galaxy presents as a somewhat elongated, lenticular or early-type spiral galaxy. It has a bright central bulge that appears smooth and featureless, indicating an older stellar population.  A very faint disk structure can be seen with low surface brightness extending from the bulge, suggesting a possible spiral arm morphology, although it is not well-defined. The colors observed indicate a mixture of stellar populations. The central region shows a yellower hue suggesting older stars, whereas the fainter outer disk appears slightly bluer, hinting at the presence of younger, hotter stars and a small amount of ongoing star formation activity. There appears to be some minor tidal disturbances, such as some faint and very short streams of light extending from the galaxy, but the overall structure remains largely undisturbed. The galaxy does not show strong indications of an active galactic nucleus or significant dust lanes. Overall, the galaxy appears to be in a relatively quiescent state, likely transitioning from a star-forming spiral to a more passive, elliptical morphology.
