The galaxy exhibits a generally smooth morphology, with a concentrated central bulge that appears somewhat elliptical. The color profile suggests an older stellar population dominating the core, evidenced by the yellowish-orange hue. A faint, diffuse disk is potentially present, indicated by the subtle greenish-blue fringe at the disk edges, which could represent areas of more recent, albeit weak, star formation activity. The overall structure doesn't show obvious signs of major disturbances or ongoing mergers, with the primary features presenting a relatively relaxed form. The galaxy's shape is neither perfectly round nor particularly elongated, falling somewhere in between, with the long axis more prominent. The light distribution is centrally concentrated.
