The galaxy appears as an elliptical type, exhibiting a smooth, diffuse morphology. The central region shows a concentrated brightness indicative of a galactic bulge. The galaxy's color profile suggests a population of older stars. A slight elongation is apparent in its shape, hinting at a cigar shaped form. There appears to be some subtle asymmetrical structure present within the faint outer regions. There's no discernible spiral arm structure, strong dust lane features, or indications of ongoing major merger activity. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or close companion galaxies. The outer regions fade gradually into the background, indicating a lack of sharp boundaries.