The galaxy presents as a single object with a relatively smooth overall appearance. It appears primarily elliptical or lenticular based on the light distribution. The core is the brightest region, exhibiting a yellowish-white hue indicative of an older stellar population. Moving outwards from the core, the galaxy shows a slight fading of intensity and a subtle color shift towards redder tones. There is evidence of some disturbed morphology within the galaxy; an interaction or minor merger seems likely. One potential tidal tail extends outwards. There is no clear spiral arm structure observed; the galaxy is primarily featureless, but also not totally spherical. It is best characterized as intermediate in shape.
