The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, appearing bright and somewhat unresolved in this image. The galaxy's overall shape leans towards an in-between roundness, showing a slight elongation. There's no obvious spiral structure or prominent dust lanes visible. Evidence of recent or ongoing major mergers is absent. The color gradient suggests a population of older stars, with a redder hue in the outer regions transitioning to bluer tones towards the core. Star formation may be present, but seems limited. Any signs of tidal tails or distortions are subtle.
