The galaxy presents as an object of moderate apparent size with a bright, concentrated central region. There is evidence of a surrounding disk component. The disk appears somewhat disturbed or irregular in form. No clear spiral arm structure is readily discernible. The galaxy exhibits a slight asymmetry in its overall shape, and there may be a minor disturbance event evident, possibly indicative of tidal interactions. The color profile reveals a relatively consistent bluish hue in the core which blends into slightly redder tones toward the outer regions, suggesting ongoing star formation.
