The galaxy presents as a moderately luminous, elongated object. It appears to be a relatively smooth galaxy with a high degree of central concentration. The color profile indicates a yellowish hue, which suggests a population of older stars. The shape deviates significantly from a perfect circle, appearing more cigar-shaped and suggesting that the object is likely either an elliptical galaxy or a spiral galaxy seen edge-on, with little to no visible spiral structure. There are no obvious signs of recent major mergers or significant tidal disturbances, but there is a slight asymmetry in the light distribution, suggesting a possible minor interaction or an internal process causing mild perturbation.
