The galaxy presents a largely smooth morphology, with a slightly elongated, though generally rounded, overall shape. There is little evidence of strong spiral arm structure or prominent disk features. The light profile appears centrally concentrated with a bright core. The color gradient suggests a population of older stars, especially in the inner regions. However, there is also some evidence of a bluer component in the outer regions. The galaxy is relatively isolated, without any obvious major tidal disturbances or close companion galaxies indicative of recent major merger events.
