The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, elliptical profile with a bright central bulge. The lack of well-defined spiral arms suggests a diminished rate of star formation and an older stellar population. Its color is generally yellowish-white, indicative of older stars. The galaxy displays some asymmetry, with one side appearing slightly more extended or disturbed than the other, indicating a possible minor interaction. Overall, it presents as a relatively quiescent galaxy nearing a state of passive evolution.
