The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. It appears to be dominated by a spheroidal component, with a gradual falloff in surface brightness from the core outwards. There is evidence of a faint disk structure, but the spheroid dominates. A notable color gradient is observed within the galaxy. The core is dominated by redder colors and is likely older stars, while the outer regions exhibit bluer colors indicative of more recent star formation activity. This is supported by its star formation rate. The image hints at minor disturbances, but these are subtle and do not significantly disrupt the overall smooth morphology. The galaxy is isolated; there are no signs of major mergers or tidal interactions.
