The galaxy presents a diffuse morphology, appearing relatively small in angular extent. The light distribution appears somewhat irregular, suggesting a system that is either undergoing interactions or possesses an ill-defined structure.

The dominant color of the galaxy is reddish, indicating a relatively older stellar population. However, localized regions exhibit a bluer hue, potentially signifying areas of more recent star formation activity. There is a faint, elongated tail-like structure extending from the main body of the galaxy, possibly evidence of tidal interactions or previous merger events. The central region of the galaxy does not display a strong, well-defined nucleus. The observed light profile suggests a gradual increase in intensity towards the center, rather than a sharp peak, pointing towards a more dispersed stellar distribution.
