The galaxy presents an overall elliptical morphology, although there is some evidence of a possible disk component. It appears relatively smooth in structure, with a centrally concentrated luminosity profile. The core of the galaxy exhibits a yellowish-white hue, suggestive of an older stellar population dominating the central region. Moving outward from the core, the color gradually shifts toward a redder tint, indicating the presence of a mixture of stellar populations with a significant fraction of older stars. A faint, extended halo surrounds the central region, contributing to the overall diffuse appearance of the galaxy. There are hints of subtle disturbances within the structure, possibly a minor interaction or past merger event. Overall, the galaxy seems to be relatively massive, with a moderate rate of star formation and is undergoing some level of interaction.
