The galaxy presents as a relatively smooth, elliptical object with a high degree of central concentration. Its morphology is largely featureless, lacking prominent spiral arms or a distinct disk structure. The galaxy appears more elongated than perfectly circular; there is a cigar shape. The color profile suggests an older stellar population, with a yellowish hue dominating the central regions, transitioning to a slightly bluer, but still subdued, halo. There is no evidence of ongoing major star formation activity. The galaxy shows no strong signs of recent or ongoing mergers or significant tidal disturbances. The overall impression is that of a mature galaxy, largely quiescent in its star-forming history.
