The galaxy presents a generally smooth appearance, with a centrally concentrated bulge that dominates the overall luminosity. The galaxy exhibits an elliptical morphology, appearing somewhat elongated along its major axis. There is a subtle transition from the bright central region to the fainter, more diffuse outer regions. No distinct spiral arm structures or prominent dust lanes are visible. The color profile suggests an older stellar population. Faint color variations may indicate some degree of ongoing or recent star formation, albeit at a low rate. There is no significant distortion of the main galactic structure or indications of major merger events. Subtle disturbances may indicate minor gravitational interactions, but these are not dramatically altering the overall structure of the galaxy.
