The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge that is brighter and more concentrated. The overall color profile appears to be skewed towards the red end of the spectrum, with the core exhibiting a pronounced yellow-orange hue. The galaxy's shape is elongated, appearing more cigar-shaped than perfectly spherical. There is no readily apparent evidence of a distinct disk structure or spiral arms, though the resolution is limited. The surrounding halo appears faint and diffuse, gradually blending into the background sky. There are no prominent signs of ongoing major mergers or tidal disturbances, though there appears to be a slight asymmetry to the outer edges. Overall, the galaxy seems to be a relatively evolved system, potentially with a low rate of current star formation.
