The galaxy presents as an elongated, cigar-shaped structure. It exhibits a central bulge with a high degree of smoothness, suggesting a relatively old stellar population. The color profile of the bulge appears more reddish, indicative of older, cooler stars. Moving outward from the central bulge, a fainter, bluer disk-like component is observed, implying the presence of more recent star formation activity. The disk does not appear to have well defined spiral arms. There is a smaller object close to the galaxy, which may be a satellite galaxy, tidal debris or background object. The overall morphology suggests this galaxy is an elliptical galaxy with a weak disk. The lack of significant distortions in the galaxy's shape suggests it has not undergone major recent mergers or interactions.
