The galaxy presents as a lenticular or possibly elliptical type, exhibiting a smooth, concentrated central bulge that diminishes gradually into a diffuse halo. Its overall morphology appears elongated, approximating a cigar shape with a high aspect ratio. The central region is a bright, yellow hue that likely indicates an older stellar population, potentially dominated by red giant stars. The outer regions transition to a dimmer, bluer coloration suggesting the presence of more recent, although limited, star formation. No distinct spiral arms or prominent dust lanes are visible within the available resolution; the overall structure appears smooth and relatively featureless. There's no apparent indication of tidal disturbances or ongoing mergers with other galaxies.