The galaxy presents a relatively smooth and elliptical morphology. The light distribution appears concentrated towards the center, indicative of a bulge component. A subtle flattening is observed, suggesting a deviation from a perfect spherical shape, and leaning towards a more disk-like structure. The color profile shows a primarily yellowish-white hue across the galaxy, possibly indicating a population of older stars. A very slight bluer tint can be observed in the outer edges of the disk. No distinct spiral arms or significant dust lanes are apparent. There is no indication of major ongoing merger events or strong tidal disturbances. The galaxy's structure suggests it is likely an intermediate type, possibly between a pure elliptical and a spiral galaxy, displaying characteristics of both. Star formation is likely limited, although a slight star formation rate may be present. The galaxy's intermediate roundness and smoothness further support its classification as potentially an early-type spiral or a late-type elliptical galaxy.
