The galaxy presents a generally elliptical morphology, appearing as a smooth, concentrated spheroid of light. The color profile suggests a mature stellar population, indicated by the yellowish-red hue, likely dominated by older, redder stars. No distinct spiral arm structures or dust lanes are discernible. The light distribution gradually decreases from the central bulge outwards. There is no significant evidence of ongoing star formation regions in this image. The galaxy displays a relatively undisturbed form, lacking apparent signs of major mergers or tidal interactions.
