The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, indicative of an older stellar population. The outer regions display a gradual decline in luminosity, with a subtle color gradient suggesting potentially younger stars or ongoing star formation, albeit at a relatively low rate. There are no discernible spiral arms or prominent dust lanes visible. The overall shape appears fairly rounded, leaning more towards spheroidal. There is no clear evidence of significant tidal disturbances or recent major merger events.
