The galaxy appears to be a relatively small, early-type galaxy, most likely an elliptical or lenticular. It exhibits a smooth, concentrated central bulge that gradually fades into an extended halo. The overall shape is somewhat elongated, but with no distinct spiral arm structures visible in this image. The color is a general yellowish-white, with a slightly bluer central region, suggesting some level of ongoing star formation, albeit at a low rate. There is no clear evidence of dust lanes or recent merger activity based on visible morphological distortions. The light distribution indicates a centrally concentrated mass distribution. Given the apparent lack of prominent features, the galaxy is likely to be relatively evolved, with a stellar population dominated by older stars.
