The galaxy presents as a relatively small, elliptical structure. It appears to have a smooth, somewhat diffuse morphology with a concentrated central bulge and a faint extended halo. The color profile suggests an older stellar population, with a dominant yellow-red hue indicative of evolved stars. There is no clear evidence of spiral arms or significant dust lanes. The shape is somewhat elongated, leaning towards a cigar shape. No major signs of ongoing mergers or tidal disturbances are immediately visible.
