The galaxy presents as a relatively smooth, centralized object with a slightly elongated shape. It lacks a distinct spiral arm structure or a prominent bulge. The central region appears brighter and more concentrated than the outer edges, which gradually fade into the background. The color profile suggests a population of older stars, with a yellowish-orange hue dominating the galaxy's light. There is little evidence of ongoing star formation, indicated by the absence of bright blue or pink regions associated with young, hot stars. Overall, the galaxy's morphology is indicative of an elliptical or lenticular type. There appear to be some minor disturbances within the galaxy, perhaps indicative of a very small merger event, but most likely there is no strong gravitational influence from any outside forces.
