The galaxy appears to be a relatively compact, early-type system, exhibiting a smooth, diffuse light distribution, with a high level of roundness. A slightly brighter central region is observed, suggesting a small galactic nucleus. The object appears nearly face-on, displaying subtle deviations from perfect circular symmetry. A faint disk structure may be present, but is largely featureless, with no resolved spiral arms or prominent dust lanes discernible. Based on its color, the galaxy is likely composed of an older stellar population, with a relatively low rate of ongoing star formation. There is no evidence of any tidal tails, strong interactions, or major mergers, suggesting the galaxy has evolved in relative isolation. The overall color index indicates a relatively red spectral energy distribution for the galaxy as a whole.
