The galaxy presents as a somewhat smooth, elliptical-like structure with a dominant central bulge. The color distribution suggests a concentration of older stellar populations, indicated by the yellowish-orange hue prominent in the core. There appears to be a slight elongation to the galaxy’s overall shape, tending toward a cigar-like form.

While appearing generally smooth, faint hints of possible disk features are present in the surrounding regions. There is no clear evidence of a major ongoing merger or significant tidal disturbances. The galaxy's color profile indicates moderate star formation.
