The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness outward from the core. The galaxy appears largely featureless, lacking any prominent spiral arms, bars, or dust lanes visible at this resolution. The color of the galaxy suggests an older stellar population, with a reddish hue indicating a prevalence of evolved stars. There is no strong evidence of on-going or recent star formation within the system based on its color and smooth morphology. The overall shape of the galaxy is roughly circular, with a slight suggestion of ellipticity. There is no obvious tidal distortion or signs of a major merger event in its recent past.
