The galaxy presents an elliptical morphology, appearing as a flattened spheroid with a smooth light distribution. The central region exhibits a concentrated, luminous core, suggesting a high stellar density. Progressing outwards, the light gradually diminishes towards the edges of the galaxy. The primary color gradient shifts from a yellowish hue at the center to a slightly redder tone in the outer regions. No distinct spiral arm structures or prominent dust lanes are apparent. The overall appearance indicates a relatively evolved system dominated by older stellar populations, with a low rate of ongoing star formation. There is a possible faint dust lane along the major axis. The galaxy does not show any visible signs of recent major merging activity.