The galaxy presents as a somewhat elliptical, diffuse object. The core appears relatively smooth, with no distinct spiral arm structures readily visible. The color profile suggests a population of older stars, with a reddish hue dominating the central regions. Faint blue tinges at the outer edges hints at some ongoing, albeit low, star formation. The galaxy exhibits a relatively high degree of roundness. There is suggestion of a possible minor gravitational disturbance with some slight irregularities in its outer regions. Overall, the galaxy appears to be relatively massive.
