This galaxy presents as a single, dominant object with a largely smooth morphology. The light is concentrated towards the center, suggesting a prominent bulge or core. The radial distribution of light indicates a fairly elliptical shape, with a high degree of central concentration. The color profile appears relatively uniform across the galaxy, which is indicative of an older stellar population. There are no obvious signs of spiral arms, dust lanes, or ongoing major merging activity. There is a slight asymmetry to the outer isophotes, possibly suggesting a past minor interaction or some internal disturbance, though these are subtle. Overall, this galaxy seems to be a relatively quiescent and evolved system.
