The galaxy presents a generally smooth, elliptical morphology. It appears relatively concentrated with light, suggesting a bulge-dominated system. The central region exhibits a bright, yellowish hue, potentially indicating an older stellar population. There is little evidence of strong spiral arms or prominent dust lanes. The light profile appears moderately rounded, with a slight deviation toward an elongated shape, although not distinctly cigar-shaped. There is no obvious indication of major disturbances from mergers or significant tidal interactions. A subtle blue tinge on the edge indicates some star formation.