The galaxy presents as a smooth, elliptical morphology. Its central bulge exhibits a concentrated, luminous profile with a yellowish hue. The isophotes display a relatively high degree of ellipticity, appearing somewhat cigar-shaped. There is no apparent evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of ongoing or recent major merger activity or tidal disturbances. The color gradient suggests an older stellar population dominating the light output, consistent with a relatively quiescent star formation rate. The size of the galaxy suggests that it is a fairly large galaxy.
