The galaxy presents as a relatively smooth, elliptical morphology with a concentration of light towards the center. There is minimal evidence of spiral arms or significant disk structure. The color appears primarily yellowish-orange, suggesting a stellar population dominated by older, redder stars and reduced active star formation. There is a slight elongation, but overall the galaxy is moderately round. No obvious signs of a major merger or tidal disturbances are visible, though a slight asymmetry may indicate minor gravitational interactions. The galaxy appears as a single, distinct entity, without clearly defined substructures or prominent dust lanes.
