The galaxy appears to be a relatively smooth, somewhat rounded system. There is an absence of clearly defined spiral arms or a prominent disk structure. The central region exhibits a higher concentration of light, suggesting a possible bulge component. Color variations are subtle, with a general trend from a slightly yellower center to bluer outer regions. There is some evidence of minor disturbances within the galaxy's structure; although, it does not appear to be undergoing a major merger event. The overall morphology suggests this galaxy may be a transitioning system, possibly between a spiral and elliptical classification. The light is fairly uniform across the galaxy's surface, suggesting a relatively stable, long-lived stellar population.
