This galaxy exhibits an overall elliptical morphology, appearing cigar-shaped in its projected form. The central region is characterized by a bright, concentrated core, potentially indicative of an older stellar population. Moving outwards from the core, the galaxy appears smoother in texture, lacking prominent spiral arm structures or distinct dust lanes. The galaxy's color profile suggests a transition from a yellowish-white core region to a bluer outer halo. This difference in color may imply varying stellar populations, with a higher proportion of older, redder stars concentrated in the center and younger, bluer stars populating the outer regions. There are signs of minor disturbances, but overall the structure appears relatively undisturbed.
