The galaxy presents as a luminous, centrally concentrated object. It exhibits a generally smooth morphology, with a notable lack of spiral arm structures or prominent dust lanes within the optical wavelengths presented. The color profile suggests an evolved stellar population, likely dominated by older, redder stars, particularly in the central bulge. There may be hints of a disk structure, though not clearly defined and the high roundness suggest this disk is face-on. Based on its features, the galaxy is likely classified as an early-type galaxy, possibly an elliptical or lenticular galaxy. The absence of strong blue colors suggests relatively low levels of ongoing star formation within the galaxy. There is no clear indication of any major ongoing mergers or tidal disturbances; however, minor irregularities cannot be ruled out given the image resolution.
