The galaxy presents as a primarily smooth object with a slightly elongated, cigar-like shape. The core region exhibits a concentrated, luminous glow, appearing brighter and more yellow than the outer regions. The light distribution suggests a spheroidal morphology, but with some asymmetry in the outer halo. There are hints of a faint, diffuse structure extending from the main body, but no obvious spiral arm features or a well-defined disk are apparent. The galaxy's color suggests a population of older stars, with a relatively low rate of ongoing star formation. There is no significant evidence of any major merger events or strong tidal disturbances.
