The galaxy appears as a centrally concentrated object, with a smooth, diffuse light distribution. Its overall shape is close to elliptical but appears somewhat elongated along a primary axis. The core region exhibits a brighter, more concentrated luminosity, possibly indicative of a bulge structure. There is no distinct spiral arm structure visible. The galaxy's color profile suggests an older stellar population, indicated by the redder hues in the central region, transitioning to slightly bluer tones in the outer regions. There may be minor disturbances visible, but the main structure appears intact, suggesting a lack of major recent merger events. Overall, the galaxy is consistent with an elliptical or lenticular type.
