The galaxy appears as a moderately bright, centrally concentrated object. Its morphology is largely smooth, with a high degree of circularity. The light profile exhibits a dominant central bulge or core, and there's a lack of discernible spiral arm structure. There is an indication of a possible minor disturbance or interaction, though the primary structure remains largely undisturbed. Color gradients are present, with a yellowish-white central region and a tendency towards redder hues in the outer regions. This may indicate an older stellar population in the galaxy's halo or disk. Overall, the system looks to be fairly massive with a relatively low star formation rate.