The galaxy presents a generally smooth morphology, appearing as a somewhat diffuse object with a radial profile. There is a slight elongation, suggesting a mild disk-like component, but the light distribution is predominantly centrally concentrated.  Based on its color, its starlight seems to be composed primarily of older, redder stars. Subtle color variations may suggest the presence of some younger, bluer stellar populations, though these are not prominent. Possible signs of disturbance can be seen, suggestive of a minor interaction.
