The galaxy presents a generally smooth and elliptical morphology. The primary body of the galaxy exhibits a concentrated central bulge, characterized by a yellowish hue, likely indicative of an older stellar population.  There appears to be a slight extension along one axis, suggesting a mild departure from perfect sphericity.  Fainter, diffuse light surrounds the central bulge, forming a faint halo or envelope.  There is little evidence of prominent spiral arms or dust lanes, lending to its smooth appearance.  Faint blue-ish tinges around the edges of the galaxy suggest very minimal recent star formation in these areas. There is no visual evidence of any major mergers or strong tidal disturbances; however, the faint asymmetry may indicate minor interactions.
