The galaxy appears to be a spiral type, albeit viewed at an angle that obscures a clear disk. The morphology is somewhat disturbed, possibly exhibiting signs of a minor interaction or tidal features. There is an irregular, diffuse shape to the galaxy. Some knotty or clumpy features are present, hinting at regions of active star formation.

The color gradient suggests a mix of stellar populations. The central region appears relatively redder, potentially indicating an older stellar population or dust obscuration. The outer regions display bluer tints, characteristic of younger, hotter stars associated with ongoing star formation. The galaxy's overall brightness is relatively moderate. The overall size is consistent with a galaxy of moderate luminosity at its estimated distance.
