This galaxy appears to be a relatively smooth object, exhibiting a dominant central bulge. The light distribution suggests a moderate concentration, transitioning from a bright, nearly stellar core outward. There is little evidence of spiral arms or significant disk structure discernible within the image. The galaxy is elongated, with a color gradient shifting from a yellowish core to a somewhat redder halo. The outer regions exhibit a gradual fade into the background, suggesting a lack of distinct boundaries. Possible minor asymmetries or disturbances are subtle and difficult to confirm at this resolution. Overall, the galaxy presents as a well-defined, likely early-type system.
