The galaxy presents a generally smooth morphology with a slight elongation. The central bulge is prominent and exhibits a concentrated, bright luminosity, suggesting a high density of stars. A faint, diffuse disk surrounds the bulge, but the disk structure is not well-defined in this image. There are indications of some subtle features or minor disturbances within the disk, with slightly asymmetric light distribution. The overall color appears to be moderately red, indicative of an older stellar population or significant dust obscuration. The galaxy does not appear to be undergoing a major merger or significant interaction, but there could be minor tidal features or distortions present upon closer inspection.
