The galaxy presents as a relatively smooth, rounded structure, appearing somewhat elliptical in form. The light distribution is centrally concentrated with a gradual decrease in intensity towards the outer regions. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region, transitioning to a slightly bluer tint at the edges. The galaxy exhibits minimal signs of significant dust lanes or spiral arm structures, indicating a lack of ongoing major star formation within the visible spectrum. There is a faint, less defined structure of a more red color to the upper left of the main galaxy structure. The galaxy's overall appearance implies a well-evolved system with a substantial stellar mass.
