The galaxy presents as a largely smooth structure with hints of a disk-like morphology. It displays an overall elliptical or nearly round shape. The galaxy exhibits a dominant central bulge, characterized by a concentrated luminosity gradient. This central region appears relatively homogenous in color, indicating a population of older stars. Fainter and more diffuse regions of less concentrated light extend from the main body, suggesting a disk component. There is minimal evidence of significant spiral arm structure or strong dust lanes, and the galaxy appears to be relatively undisturbed, showing no obvious signs of a major merger event. Subtle color variations suggest some ongoing star formation, but this activity is most likely at a relatively low rate.
