The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated luminosity, gradually decreasing towards the outer edges. The color profile suggests a dominant population of older stars, inferred from its reddish hue, with a hint of younger, bluer stars interspersed throughout, contributing to a slight greenish-yellow tint. There are no immediately discernible spiral arms or prominent dust lanes. The galaxy appears well-defined, showing no major signs of significant tidal disturbance or ongoing major merger activity. A minor asymmetry or potential interaction with a smaller, less luminous object is not definitively ruled out. The overall shape appears to be consistently rounded.
