The galaxy presents as a somewhat flattened spheroid, with an overall smooth appearance. The central region exhibits higher surface brightness, appearing more luminous and concentrated than the outer regions. There is a subtle color gradient, with the central bulge trending towards bluer wavelengths compared to the more muted hues of the surrounding halo. No distinct spiral arm structures or prominent dust lanes are discernible. There is a slight indication of minor disturbances present in its overall structure, but this is not overtly pronounced. The galaxy does not appear to be undergoing a major merging event or significant tidal interaction.
