The galaxy presents a generally smooth morphology, appearing elliptical in shape. It exhibits a prominent central bulge, concentrated and luminous, with a yellowish-orange hue. The outer regions of the galaxy are less defined, gradually fading into the background. A slight elongation is observed, suggesting it is not perfectly spherical, perhaps closer to a cigar shape. There is no discernible spiral arm structure or obvious dust lane features visible within the galaxy. The overall color profile suggests a population of older stars. No significant signs of ongoing major merger activity, such as tidal tails or strongly distorted morphology, are immediately apparent, although there may be minor disturbance present.
