The galaxy presents as a relatively compact, elliptical structure. The light distribution is centrally concentrated, exhibiting a smooth gradient outwards from a brighter core. The galaxy's shape is elongated, showing a clear deviation from a perfect circle, tending toward a slightly cigar-shaped form. There is some subtle suggestion of internal structure, but the overall impression is of a relatively homogenous light profile, with an absence of pronounced spiral arms or distinct star-forming regions. There is a hint of a disk feature. The color appears moderately red, with an overall distribution indicating a population of older stars with little current star formation. There is no strong evidence of tidal tails or other indications of recent major mergers or significant gravitational disturbances.
