The galaxy presents as a relatively compact and moderately luminous object with an elliptical or lenticular morphology. Its core is a diffuse, concentrated region that appears smooth in texture. The galaxy exhibits a notable lack of distinct spiral arm structures, with no evidence of a prominent disk. Its color appears to be a yellowish-orange, suggesting an older stellar population and reduced ongoing star formation activity. There is potentially a hint of minor tidal disturbance or faint structure extending beyond the main body, though the low resolution makes it difficult to confirm the presence of any active merging events.
