This galaxy exhibits a complex morphology, appearing neither purely elliptical nor a well-defined spiral. There is evidence of a disturbed structure, possibly indicative of an ongoing or recent interaction. Patches of diffuse light are visible, with a central region of slightly higher surface brightness.

The galaxy displays a range of colors. Bluish hues are scattered throughout the galaxy, perhaps indicating regions of active star formation. Some areas show a shift toward redder tones, which could suggest older stellar populations or dust obscuration. The overall color profile is relatively heterogeneous across the galaxy's extent. The distribution of light is somewhat irregular, and there appear to be streams or tidal tails extending from the main body. These features might be the result of gravitational interactions with another galaxy. The galaxy's estimated size is small.
