The galaxy presents as a moderately luminous, elliptical galaxy. Its shape is elongated, appearing cigar-shaped rather than perfectly spherical. The light profile suggests a centrally concentrated bulge that fades smoothly outward, characteristic of elliptical galaxies. There is no indication of spiral arms or a prominent disk structure. The color is generally yellowish, indicating an older stellar population dominated by redder stars, consistent with a relatively low star formation rate. There is no evidence of strong tidal features, major disturbances, or ongoing mergers, suggesting that the galaxy is relatively isolated and undisturbed.
