The galaxy presents as a relatively smooth, elliptical-like structure. The color profile indicates a dominant population of older stars, characterized by a yellow/orange hue, especially in the central region. There is some indication of bluer light towards the outer edges, suggesting the possibility of younger star formation, albeit at a lower rate compared to actively star-forming galaxies. The galaxy appears somewhat elongated, showing an axial ratio greater than one, implying that it is not a perfect sphere. The light is concentrated towards the center, with a gradual falloff toward the edges, indicative of a spheroidal distribution of stars. No distinct spiral arms or prominent dust lanes are visible. There are no obvious signs of a recent or ongoing major merger event. However, subtle irregularities in the light distribution suggest the possibility of a past minor interaction or accretion event.
