The galaxy presents a somewhat elliptical morphology, exhibiting a relatively smooth appearance. It appears to have some central concentration of luminosity, with the light gradually fading towards the edges. There is a slight elongation visible, suggesting it may be transitioning from a spherical to a more lenticular or disc-like form. The light is redshifted, indicating significant distance. The color is generally consistent throughout, trending towards the redder end of the spectrum, which, combined with the smoothness, hints at a population dominated by older stars. There are subtle indications of minor disturbances, but the overall structure appears largely undisturbed.
