The galaxy presents as a relatively smooth, elliptical form. There is a slight elongation, approximately cigar-shaped. A small hint of internal structure can be seen, but overall it exhibits a fairly uniform surface brightness profile across its main body, with no prominent spiral arms or bar structures visible. It appears to be a relatively quiescent galaxy with a low star formation rate, suggesting a population dominated by older stars. There is no evidence of major mergers or significant tidal disturbances, but some degree of minor interaction cannot be fully ruled out based on this single image. The color suggests a typical elliptical galaxy population of older stars, with a reddish hue, consistent with it being relatively massive.
