The galaxy presents as a moderately luminous object with a discernible structure indicative of ongoing interaction or disturbance. At its core is a relatively bright, concentrated region which appears yellowish-orange in color. This core is surrounded by a less concentrated, more diffuse halo of bluish light, suggesting the presence of a younger stellar population and recent star formation.

The overall shape is somewhat irregular, lacking a well-defined spiral or elliptical morphology. There are apparent distortions and extensions of luminous material extending outwards from the central region. These features suggest possible tidal interactions with another galaxy, or perhaps internal processes disrupting its morphology. There is also a hint of filamentary structure emanating from the core region, hinting at the possibility of past or ongoing merger events.
