The galaxy presents an elliptical morphology, appearing largely smooth and centralized. A bright, concentrated core region is visible, indicating a higher density of stars and potentially the presence of a supermassive black hole at the galactic center. The light profile decreases gradually from the core outwards. There is subtle color variation present, with the central region exhibiting a yellowish hue. This suggests an older stellar population, while the outer edges show slight tinges of bluer tones. However, the overall color profile indicates a lack of significant ongoing star formation across the galaxy. There are some minor asymmetric disturbances in the shape of the galaxy, with a slightly jagged edge on the bottom left of the galactic disk. This may indicate that the galaxy is potentially in the early stages of a minor merger event with another smaller galaxy. No distinct spiral arms or prominent dust lanes are observed within the galaxy, consistent with the overall smooth appearance.
