The galaxy presents as a relatively small, smooth object with a nearly circular morphology. The primary color is a noticeable blue-green hue, indicating the likely presence of relatively young, hot stars. The light is quite concentrated toward the center of the galaxy, suggesting a possible central bulge or active galactic nucleus, though detailed spectral analysis would be required to confirm this. There appears to be a very slight distortion or minor disturbance in the overall structure, possibly caused by a past or ongoing gravitational interaction with a companion galaxy. No prominent spiral arms or other distinct features are immediately apparent, consistent with a possible elliptical classification, though further investigation is required for conclusive classification. Overall, the galaxy exhibits characteristics of a compact, possibly actively star-forming, early-type galaxy.
