The galaxy appears as a centrally concentrated object, exhibiting a largely smooth, elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes within the galaxy itself. The color appears mostly homogenous, with a dominant yellow hue, suggesting a stellar population primarily composed of older stars. The galaxy appears to be reasonably round, with some light suggesting that it may be slightly cigar-shaped. There do not appear to be any significant tidal features or nearby companions to suggest recent or ongoing major mergers. There is evidence of some minor disturbances, though these are not very significant. The galaxy lacks obvious signs of active star formation regions within the central region.
