The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's overall structure. The light distribution appears relatively even and diffuse, with no prominent spiral arms or dust lanes visible at this resolution. The galaxy appears moderately rounded. A slight elongation may be present, although it's subtle. There appear to be no signs of significant tidal disturbances, strong asymmetries, or a recent major merger event. The color indices suggest a population of older stars, contributing to the redder overall hue. The star formation rate is relatively low, possibly indicating a galaxy nearing the end of its active star-forming phase.
