The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, relatively featureless morphology. Its color profile indicates a population of older stars, as suggested by the yellowish-red hue, indicating that star formation activity is likely subdued. There is no obvious spiral arm structure or dust lane features, instead a somewhat diffuse and uniform light distribution is present. The galaxy appears somewhat elongated, more so than perfectly round, but not significantly cigar shaped. There is no obvious evidence of a major merger or significant tidal disturbances in its immediate environment. Light profile is centrally concentrated, with brightness falling off with radial distance from the center of the galaxy. There may be low level star formation in the galaxy. 
