This galaxy appears to be an elliptical type, exhibiting a generally smooth and featureless morphology. The light distribution is centrally concentrated, with a bright, compact core that fades into a more diffuse outer region. The overall shape is elongated, approximating a cigar shape, suggesting some degree of flattening, though not to the extent expected in a spiral galaxy. There is no obvious dust lane or spiral arm structure visible. The color profile is largely yellow-red, indicative of a population dominated by older stars and a low rate of ongoing star formation. There is no evidence of any major mergers or tidal disturbances, though some minor disturbances are not entirely ruled out based on the shape of the galaxy.
