The galaxy exhibits a generally elliptical morphology, appearing smooth and relatively featureless. The light distribution shows a strong central concentration, indicated by a bright, yellowish core that gradually fades toward the outer regions. There is a slight elongation visible, suggesting that the galaxy is not perfectly spherical. The overall color profile appears to be dominated by older stellar populations, evident from the yellowish hue, with a lack of prominent blue regions indicating subdued current star formation activity. There is a possible faint disk component that can be seen perpendicular to the elongated axis. There are no clear signs of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed within its immediate environment.
