The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical in projection. The galaxy displays a yellowish hue, suggesting a population dominated by older stars. There are no apparent spiral arm structures or significant dust lanes. The galaxy appears relatively isolated, with no immediate signs of ongoing major merger activity or significant tidal distortions. A faint, diffuse halo is suspected but not clearly visible. The object likely has minimal star formation activity. Overall, this appears to be a mature elliptical galaxy with little ongoing star formation.
