The galaxy exhibits an overall elliptical morphology. A bright, concentrated central bulge dominates the visual appearance. The galaxy appears to be relatively smooth, with a fraction of the galaxy shape being more feature-like or disk-like. A faint halo surrounds the bulge, extending further along a preferred axis. The distribution of light suggests an intermediate stage in the transition from a spiral to a fully elliptical galaxy, with the remaining disk features not being as prominent. The color gradient indicates a higher concentration of older stellar populations within the central bulge, with a less active star formation rate overall. The galaxy's shape is observed as somewhat elongated, resembling a cigar shape. There are no evident signs of tidal disturbances or ongoing major mergers, but there may be minor disturbances.
