This galaxy presents a generally smooth, elliptical morphology with an approximate physical radius of 5.9 kpc. The light profile is highly concentrated toward the center, with a bright, unresolved core. The galaxy exhibits a yellow-red color, consistent with an older stellar population. There is no apparent spiral arm structure or evidence of significant dust lanes. Based on its apparent roundness, the galaxy appears closer to spherical than disk-like. There are no obvious signs of a major ongoing merger or tidal interactions, although some minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively quiescent system with a low star formation rate.
