The galaxy presents as a moderately bright, elliptical form with a relatively smooth, featureless appearance. It exhibits a noticeable color gradient, transitioning from a warmer, yellower hue near the central region to cooler, bluer tones in its outer edges. The shape is elongated, displaying a cigar-like, oblong structure rather than a perfectly circular or spiral organization. There's no obvious sign of major disturbances or ongoing merging activity. The central bulge appears prominent, indicating a likely significant concentration of older stellar populations in that region. The outer regions display a fainter, more diffuse halo, possibly indicating older stars. Despite the color gradient, the lack of well-defined spiral arms or dust lanes suggests a low current star formation rate.