The galaxy presents as a relatively smooth object, showing a slight concentration of light towards the center, with a more diffuse outer region. It is generally elliptical in appearance but leaning to the rounder side, with no obvious spiral arm structures or bar features visible. The light distribution suggests a relatively uniform stellar population, with no strong indication of ongoing major star formation regions. There might be some minor evidence of a slight disturbance within the galaxy, although it is hard to definitively say, but it does appear as though it could have minor merging properties. The galaxy's color appears to be somewhat red, indicating a population of older stars and a low current star formation rate. Its apparent physical size suggests a moderate sized galaxy.
