The galaxy appears as a relatively compact and luminous object. Its overall morphology is generally smooth, with a hint of some internal structure, potentially hinting at a very faint disk or arm features. The light distribution suggests a centrally concentrated bulge. The color profile is interesting, with the core exhibiting a yellowish hue, which might indicate an older stellar population or the presence of dust obscuration. The outer regions display a bluer tinge, potentially revealing younger stars or less dust. There is a noticeable asymmetry to the distribution of light within the galaxy, which could be indicative of a past or ongoing minor interaction or disturbance. The object does not present a grand design spiral or a clearly elliptical shape, rather something in between. Possible tidal features are not immediately apparent.
