The galaxy presents as a relatively compact object with a centrally concentrated bulge. The bulge exhibits a smooth, yellowish-orange hue, indicative of an older stellar population. Extending from the central region are faint, diffuse features exhibiting a bluish tint, suggesting the presence of younger, hotter stars and possibly ongoing star formation. These fainter regions appear somewhat disturbed, showing irregular structures. The overall shape is neither perfectly spherical nor a well-defined disk; rather, it appears to be an intermediate form. Evidence suggests the possibility of a minor interaction or merger event in the past. The galaxy's relatively small size and smooth central component suggest it is a galaxy with an intermediate mass.
