The galaxy presents as a centrally concentrated, relatively smooth object. Its overall shape is broadly elliptical, tending towards round rather than highly elongated. A discernible color gradient is present, with the core region exhibiting a yellowish hue, potentially indicative of an older stellar population. The outer regions of the galaxy display a faint, diffuse halo with a slightly bluer tint, suggesting the presence of younger, hotter stars, although star formation activity appears generally low. There is no strong evidence of significant spiral arm structure or bar features. The galaxy does not appear to be undergoing any major mergers or experiencing significant tidal disturbances.
