The galaxy presents a generally smooth, elliptical morphology, exhibiting a centrally concentrated luminosity profile. The core region appears bright and largely featureless. Progressing outwards from the center, the luminosity decreases gradually, suggesting a diffuse stellar halo. The galaxy exhibits an overall elongated shape, appearing somewhat cigar-shaped. There is a faint bluish tint to the outer regions of the galaxy, possibly indicating some level of ongoing star formation. No prominent spiral arms or significant dust lanes are discernible, suggesting a relatively quiescent state. There appears to be no evidence of any major mergers or significant tidal disturbances.