The galaxy presents as a luminous, centrally concentrated object, exhibiting a morphology suggestive of an elliptical galaxy. Its shape is moderately elongated, deviating slightly from a perfect circle. The central region displays a high surface brightness, indicating a dense concentration of stars. The light appears to be homogenous and smoothly distributed. A faint, diffuse halo or extension of light is observed surrounding the main body of the galaxy. A fainter, smaller apparent object is visible nearby which may be a smaller galaxy or cluster of stars distorted through gravitational interaction. Despite this potential interaction, there are no obvious indications of tidal tails or other major distortions within the main body. The color suggests a stellar population dominated by older, redder stars.