The galaxy presents an elliptical morphology, exhibiting a generally smooth appearance with a concentrated central bulge. The color profile appears to be predominantly yellow, suggesting an older stellar population. The galaxy is elongated, with an approximate axis ratio of 1:3. No distinct spiral arm structures are observed. There might be a very slight disturbance or irregularity in the outer regions, but no major signs of ongoing merging events are apparent. The overall structure points towards an evolved system with a limited amount of recent star formation activity.
