The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity, indicative of a substantial stellar population. The color profile suggests a population dominated by older stars with a redder hue in the central region, possibly indicating a higher metallicity. There's an indication of a slight color gradient, transitioning to a somewhat bluer periphery, which could be due to a younger stellar population and ongoing star formation in the outer regions. There appears to be no prominent disk structure, spiral arms, or significant dust lanes visible within the resolution of the image. The galaxy shows no signs of recent or ongoing major merger activity, appearing mostly undisturbed.
