The galaxy presents a generally elliptical morphology, characterized by a smooth and concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. Extending from the main body, a discernible feature emerges, possibly indicative of a tidal tail or a disrupted arm. This feature displays a reddish coloration, potentially signifying ongoing star formation or dust obscuration within that region. The overall roundness of the galaxy points towards a relaxed system. However, the presence of the reddish feature indicates a possible interaction or past merger event, introducing some level of disturbance to its structure. The apparent smoothness and lack of distinct spiral arms would suggest that the galaxy does not have well defined spiral structure.
