The galaxy appears to be a relatively compact object. The light distribution suggests a smooth morphology, lacking prominent spiral arms or a distinct central bulge. The overall shape is more elliptical than circular, appearing somewhat elongated, but not significantly cigar-shaped. 

There is no strong visual evidence of a major merger or significant tidal disturbances, though subtle irregularities might be present upon closer inspection. The galaxy's color suggests a population of older stars, given its redder hue, but with some blue star formation in the center.
