The galaxy presents as an elliptical structure, elongated along its major axis, displaying a smooth, featureless morphology. There is no apparent spiral arm structure visible. The light distribution appears to be centrally concentrated, with the highest intensity near the core region, gradually fading towards the outer edges. The color profile suggests the presence of an older stellar population, indicated by the yellow-reddish hue, with a slightly bluer tint. The overall shape is somewhat cigar-shaped, appearing close to being edge-on relative to our line of sight. No signs of any ongoing major merger events are observed; however, minor disturbances in the outer regions cannot be definitively ruled out given the image resolution.
