This galaxy presents a morphology that is largely smooth and elliptical in appearance, with a noticeable elongation suggestive of a cigar shape. The galaxy's color profile indicates a dominant population of older stars, exhibiting a yellowish hue concentrated towards the core, with the implication of less active star formation within the galaxy. While no signs of strong tidal disturbances or ongoing major mergers are apparent in this single image, the elongated shape hints at possible past interactions or minor disturbances. There does not appear to be a defined disk or spiral arm structure.
