The galaxy appears as a moderately bright, somewhat diffuse object. It presents with an elliptical morphology, exhibiting a smooth light distribution that suggests a relatively old stellar population. The colour profile indicates a redder overall hue, typical of galaxies with lower rates of star formation. There is a faint suggestion of a slight distortion, indicating possible past or ongoing gravitational interaction with another galaxy. There is no clear evidence of spiral arms or a prominent disk structure; the galaxy appears largely spheroidal. The nucleus is subtly brighter than the surrounding regions, however there is not much dust or activity evident in the core. Overall, the observed characteristics are consistent with those of an early-type galaxy.
