The galaxy presents as a somewhat elliptical object with a bright, concentrated central bulge. There is a noticeable disk component, although it appears disturbed or irregular in shape, showing evidence of possible tidal features.

The central region exhibits a yellowish-white hue, likely indicating an older stellar population. Moving outwards from the center, there is a transition towards a reddish color, which could be due to a combination of dust extinction and the presence of older, redder stars.

The galaxy does not appear to have well-defined spiral arms. Patches of bluer light are observed, hinting at regions of recent or ongoing star formation, although they are not prominent. The overall structure suggests the possibility of a past or ongoing interaction or merger event.
