The galaxy presents as a smooth, elongated structure. Its overall shape is cigar-shaped, displaying a relatively high degree of ellipticity. The central region exhibits a concentrated, bright core, gradually decreasing in luminosity towards the outer edges. The color profile suggests an older stellar population, exhibiting a yellowish-red hue, particularly pronounced in the central bulge. There is little evidence of distinct spiral arms or active star formation regions. The morphology appears largely undisturbed, with no signs of significant mergers or tidal interactions. The light distribution suggests a fairly uniform stellar density, consistent with an elliptical galaxy classification.
