The galaxy presents a generally smooth and rounded morphology. Its color profile indicates a predominantly older stellar population, with a concentration of light towards the redder end of the spectrum. The central region appears brighter and more condensed than the outer regions, exhibiting a yellowish-orange hue. There is a notable lack of distinct spiral arm structures or prominent dust lanes. The absence of significant blue light suggests relatively low current star formation activity. Faint extensions of the galaxy can be observed gradually fading into the background sky, but there is no evidence of significant tidal disturbances or ongoing major mergers. It exhibits a fairly symmetrical shape, with no strong indications of asymmetry.
