The galaxy presents as a somewhat rounded object with a smooth, diffuse light distribution across the core. There is a slightly elongated morphology. There is evidence of a faint disk component, but no distinct spiral arm structure or bar feature is discernible. The galaxy exhibits a yellowish hue, possibly indicative of an older stellar population. There is evidence of potential merging or tidal interaction with other objects in its vicinity. Some blue areas are visible, potentially indicative of star forming regions.