The galaxy appears as a moderately bright, compact object exhibiting a relatively smooth morphology. It presents a somewhat elliptical shape, showing a structure somewhere between a perfect sphere and a more elongated form. The light distribution is concentrated, with the central region appearing brighter and gradually fading towards the outer edges. The color profile suggests a possible redder hue, particularly in the core. There is no apparent evidence of spiral arms, distinct features, or significant signs of ongoing merging activity. There are suggestions of a minor interaction or a potential companion, based on the slight asymmetry in the light distribution.
