The galaxy presents a generally smooth morphology, appearing largely featureless in this image. The light distribution suggests an elliptical or lenticular galaxy type. The galaxy exhibits a central concentration of light that gradually fades into the outer regions. The shape appears to be slightly elongated. There is no obvious evidence of spiral arms or a distinct disk structure in this observation. The color profile indicates a population of older stars dominating the light output. This galaxy shows little sign of ongoing major merger activity or significant tidal disturbances.
