The galaxy presents a generally elliptical morphology, appearing significantly elongated in shape. Its light distribution is relatively smooth, without distinct spiral arm structures visible. The core region appears slightly more concentrated, with a gradual decrease in surface brightness towards the outer edges. The color profile suggests a population of older stars dominating the overall light output, with a hint of bluer regions that could indicate some presence of younger stellar populations or active star formation, though limited. There is no evidence of significant ongoing merger activity or tidal disturbances in the image.
