The galaxy presents as a largely smooth, elliptical or lenticular structure. There is a concentrated central bulge that transitions smoothly into the outer regions. There is a noticeable lack of spiral arm structures or distinct dust lanes. The color profile appears to be predominantly yellow or orange, suggesting an older stellar population with fewer hot, young stars. There is no obvious sign of tidal tails or other significant morphological disturbances indicative of recent major mergers or interactions. Faint extensions or a very subtle halo might exist, but the resolution makes a definitive assessment difficult. Overall the galaxy presents as a relatively quiescent system.
