The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region, appearing orange-red in color, suggestive of an older stellar population. Surrounding the bulge is a less defined, somewhat diffuse disk. The disk structure appears mostly homogenous, with faint hints of a spiral structure. The disk region displays a bluer color, possibly indicating the presence of younger, hotter stars and ongoing star formation activity. There are no obvious signs of significant tidal disturbances or interactions with other galaxies, indicating relative isolation. Overall, it appears as an early type disk galaxy undergoing a period of slow star formation.
