The galaxy presents a generally smooth, elliptical morphology. It appears nearly round, with a slight suggestion of ellipticity. The light profile exhibits a concentrated central bulge that gradually diffuses into the outer regions, with no distinct spiral arm structures or prominent features visible. The color gradient is subtle, with a slightly bluer hue in the outer regions compared to the more yellow-white central bulge. The overall appearance indicates a system dominated by an older stellar population, potentially with ongoing, though relatively low, star formation activity. There are no indications of any major mergers or significant tidal disturbances.
