The galaxy presents as a single, fairly smooth object with a concentrated central region. It exhibits an elliptical morphology and a yellow hue, possibly indicating a population of older stars and a lack of significant ongoing star formation, although some is expected. The isophotes appear mostly regular, with no signs of strong tidal disturbances or ongoing major mergers. There is a slight elongation, though the galaxy appears largely round. The object's moderate estimated size suggests a typical, fairly compact galaxy. The color profile indicates a redder population with an older stellar age. The mass estimate appears to be normal for a galaxy of this type, and the star formation rate is low, though non-negligible.
