The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its light is predominantly distributed in a diffuse manner, indicating a lack of prominent spiral arms or strong dust lanes. The color profile appears to be on the redder side, suggesting an older stellar population and diminished ongoing star formation. There is a suggestion of a minor disturbance to the main galactic body, possibly due to a small interaction with a neighbor. The galaxy appears mostly undisturbed and not undergoing any major merging events.
