The galaxy presents a slightly irregular, somewhat rounded morphology. The light distribution appears centrally concentrated, suggesting a dominant bulge component. There is evidence of a possible ongoing or recent merger event given the presence of distinct luminous knots and possible tidal features or minor disturbances within the galaxy's halo. The galaxy exhibits a color gradient, with a reddish central region potentially indicative of an older stellar population or dust obscuration. Some features suggestive of a faint, bluer disc are visible. The overall color profile suggests a relatively evolved galaxy, though not entirely quiescent in terms of star formation.
