The galaxy presents as a smooth, elliptical morphology with a concentrated central bulge that emits strongly in the yellow-orange wavelengths, suggesting an older stellar population. It displays no distinct spiral arm structures or dust lanes. The galaxy has an estimated effective radius of approximately 3 kpc. There appears to be a very slight disk structure around the center. Faint diffuse light emanates from the outer regions, gradually fading into the background. The lack of prominent features implies it is likely a relatively evolved system, perhaps nearing the quiescent stage of its life cycle. There appears to be no major signs of any recent interactions or mergers.
