The galaxy appears as a relatively small, flattened elliptical shape, indicative of a disk galaxy viewed at a high inclination angle. Its light profile suggests a bright, compact central bulge with a surrounding, less concentrated disk component.

Color analysis reveals a complex structure. The central region exhibits a bluer hue, potentially indicating ongoing star formation or a population of hot, young stars. This bluer region is surrounded by a ring of green and yellow colored material, possibly indicative of dust and older stellar populations. The disk appears more uniformly red, characteristic of an older, more evolved stellar population and lower levels of star formation.

There are no obvious spiral arm structures visible. The overall structure suggests a relatively undisturbed system, free from major ongoing mergers or tidal interactions. Further spectroscopic analysis is required to confirm the stellar populations and star formation rates.
