The galaxy appears to be a relatively compact system, exhibiting a largely smooth and somewhat round morphology. A central concentration of light is evident, suggesting a possible galactic bulge or active galactic nucleus, although the resolution is insufficient to confirm this. The color profile indicates a population of older stars, as inferred from the relatively redder hues. There is a hint of some irregular structure. There does not appear to be evidence of active star formation. It might be experiencing, or approaching, a state of quiescence in terms of star formation activity. Based on the light distribution, the galaxy seems to be relatively isolated.
