The galaxy appears as a relatively small, elliptical structure with a smooth, centrally concentrated light distribution. Its color profile shows a dominant reddish-yellow hue in the central region, suggesting an older stellar population. Fainter bluish tints surround the primary disk of the galaxy and indicate younger stellar populations. There is a presence of a central bulge; however, evidence of a disk component appears absent. No spiral arm structures or dust lanes are discernible within the observable features. The absence of significant tidal distortions or nearby companion galaxies suggests that it may not be undergoing any major mergers or strong interactions. This galaxy may possess a relatively low star formation rate.
