The galaxy presents as a diffuse, elliptical structure. The light distribution appears smooth and centrally concentrated, exhibiting a noticeable radial color gradient. The core region is characterized by a distinct yellow-orange hue, suggestive of an older stellar population. Moving outward from the center, the galaxy gradually fades into a fainter, redder halo. There is no discernible spiral structure or evidence of ongoing, significant star formation activity. The morphology is indicative of a quiescent galaxy, potentially an early-type system with minimal gas content. No signs of tidal disruption or interactions with other galaxies are immediately apparent, though higher resolution data would be necessary to fully assess this.
