The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution is dominated by older stellar populations, evident by the yellowish-red hue of the core. There is a general lack of distinct spiral arm structure or prominent dust lanes. The galaxy exhibits a generally round morphology. There's a faint, diffuse halo extending beyond the central region, gradually fading into the background. No signs of major mergers or significant tidal disturbances are immediately apparent. The galaxy likely has minimal ongoing star formation based on its color.
