The galaxy appears as a centrally concentrated object with a relatively diffuse and extended halo. The core region exhibits a brighter, somewhat amorphous structure, showing evidence of potential substructure or clumping. The overall morphology seems to lean towards a disturbed or irregular shape rather than a well-defined spiral or elliptical form. There is a suggestion of tidal features, possibly indicative of an interaction or merger event. Color variations within the galaxy indicate differing stellar populations or dust content, with a slightly bluer hue in certain regions and a redder hue in others. The outer regions of the galaxy are faint and indistinct, gradually fading into the background sky.
