The object appears to be a galaxy, exhibiting a generally smooth and rounded morphology. The light profile indicates a centrally concentrated bulge. There is a faint hint of a disk extending beyond the central bulge, though it lacks distinct spiral arms. The galaxy's overall color appears relatively red, suggesting an older stellar population and potentially suppressed recent star formation. There is no significant evidence of tidal disturbances or ongoing major mergers. The galaxy's moderate size and luminosity suggest a classification as an intermediate-mass system. 
