The galaxy presents as a generally smooth object with a largely elliptical morphology. There is little indication of significant spiral arm structure. The galaxy appears to be quite round with only minor deviations from a perfect circle, perhaps a slightly more cigar-shaped form. The color gradient suggests a population of older stars, potentially indicating relatively low current star formation. There are small areas of color change and possibly dust lanes, suggesting minor disturbances or mergers. The overall luminosity suggests a relatively high mass system.
