The galaxy presents as a somewhat elongated, yet centrally concentrated object. Its light profile appears smooth, lacking any readily discernible spiral arm structure or prominent dust lanes. The core region is a yellowish-orange, potentially indicating an older stellar population and a lack of significant ongoing star formation in the central bulge. Moving outwards from the center, the color shifts towards a bluer hue, particularly at the periphery. This could suggest a population of younger, hotter stars in the outer regions of the galaxy, albeit not in significant quantities. The overall morphology suggests a galaxy that is tending towards a lenticular or early-type spiral classification, with a relatively large bulge component. There is some subtle evidence of minor tidal disturbances or interactions, perhaps an indication of past or ongoing interaction.
