The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution with no readily apparent spiral arm structure. The core appears bright and concentrated, diminishing gradually towards the outer edges. There is a slight elongation to the galaxy's shape. The color profile suggests an older stellar population, with light tending towards the redder end of the spectrum. No prominent dust lanes or regions of active star formation are visually discernible within the body of the galaxy itself, suggestive of relatively low ongoing star formation activity. No significant morphological distortions that would indicate a recent or ongoing merger are present.