The galaxy appears as an elongated, cigar-shaped structure. Its color profile suggests a relatively old stellar population, with a dominant reddish-orange hue emanating from the central bulge. There is a smooth texture. The central region is brighter than the outer regions, indicating a concentration of stars or possibly an active galactic nucleus, although the resolution does not allow for confirmation of the latter. No distinct spiral arms or dust lanes are discernible; the galaxy's overall morphology is smooth. The galaxy appears undisturbed, lacking evidence of major mergers or tidal interactions. The shape suggests that it is elliptical.
