The galaxy presents as a moderately bright, relatively compact object, with an elliptical morphology. The galactic profile exhibits a high degree of central concentration, with a gradual decrease in luminosity towards the outer edges. The isophotes appear to be moderately flattened. There is no discernible spiral arm structure. The galaxy appears to be a relatively smooth system, lacking prominent dust lanes or star-forming regions, suggesting an older stellar population with limited ongoing star formation. The overall color index indicates a preference towards redder wavelengths. The galaxy may be a member of a small group or cluster of galaxies, based on its close proximity with other galaxies in the image.
