The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The color profile suggests a dominant population of older stars, indicated by the yellowish hue of the central bulge. The galaxy appears largely spheroidal, with only subtle deviations from perfect roundness. There is little indication of prominent spiral arms or significant dust lanes within the visible structure. Faint, extended emission surrounds the core, gradually fading into the background sky. No strong tidal features or signs of a recent major merger are discernible. There are some signs of subtle disturbances but its generally relaxed morphology suggests it has not experienced significant interactions recently.
