The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a concentrated and bright yellowish-white hue, indicative of an older stellar population. Moving outward from the central region, the color gradually shifts towards a more orange-red tone, suggesting a possible presence of dust lanes and a slightly younger stellar population. The shape appears to be elongated, exhibiting an intermediate form between perfectly round and cigar-shaped. While the galaxy displays a general smoothness, there are subtle indications of possible minor disturbances or asymmetries in the outer regions. There is an apparent low level of star formation activity, possibly with very little gas, as indicated by the faint red color.