The galaxy presents a predominantly smooth, elliptical morphology. A concentrated, bright central bulge dominates the visual structure, exhibiting a high degree of radial symmetry. Fainter, diffuse light extends outward from the bulge, gradually fading into the background. There's a hint of a possible disk-like structure, though it is not well-defined. The galaxy appears moderately rounded. There is no obvious evidence of strong tidal features or ongoing major merger activity. Minor disturbances could be present within the disk, but nothing stands out as a strong interaction or merger. The galaxy displays a blueish colour, although some regions closer to the core appear more reddish. The estimated effective radius of the galaxy is approximately 4 kpc. Given the light distribution, the stellar population is likely dominated by older stars in the bulge, with some fraction of younger stars in the faint disk component, suggesting ongoing star formation.
