The galaxy presents a generally smooth morphology, exhibiting a concentrated central region with a radial decrease in luminosity outwards. The core displays a yellowish hue, indicative of an older stellar population. Moving outward from the core, the color transitions to a more greenish-white. There is no discernible spiral arm structure or bar feature. The overall shape appears elliptical, though not perfectly round, with a slight elongation. There may be signs of minor disturbances in the outer region, perhaps the result of a past merger.
