The galaxy presents a predominantly smooth morphology. There is a lack of defined spiral arms or a distinct disk structure. The light distribution appears concentrated towards the center, indicative of a bulge. The overall shape is generally elliptical, with a slight deviation from perfect sphericity. There is a hint of some structure, but it is mostly dominated by the smoother bulge. The galaxy exhibits some color variation, shifting from a possible blueish hue near the edges to a more yellow-reddish central concentration. This color gradient might imply differences in stellar populations across the galaxy, with potentially younger, bluer stars populating the outer regions and older, redder stars residing in the bulge. There is no obvious presence of strong dust lanes or active star-forming regions. Based on these traits, the galaxy appears to be an early-type galaxy, possibly an elliptical galaxy. The lack of significant distortions suggests the galaxy is not undergoing a major merger event, however there seems to be a minor disturbance.
