The galaxy exhibits a discernible disk structure, although the morphology appears somewhat disturbed. There is evidence of a relatively smooth central bulge. A notable color gradient is present, shifting from bluer hues in one region to warmer, reddish tones in another, indicative of varying stellar populations or dust content. The spatial distribution of light suggests ongoing or recent star formation activity. It appears that a potential minor merger or tidal interaction has taken place, disrupting some of the structure. Overall, the galaxy presents characteristics intermediate between a classical elliptical and a well-defined spiral, potentially undergoing a transformative process influenced by environmental interactions.
