This galaxy presents as an elongated, cigar-shaped structure. Its light profile suggests a relatively smooth distribution, with a concentrated central bulge that gradually diffuses outwards. The core exhibits a yellowish-white hue, possibly indicating an older stellar population. Fainter, bluer tints are discernible in the outer regions. No prominent spiral arms are detected. Based on its morphology and color, this galaxy is likely an elliptical galaxy. There are no apparent signs of ongoing major mergers. However, given the slight irregularities in the outer halo, the possibility of minor tidal interactions cannot be completely ruled out.
