The galaxy presents as a relatively smooth, elliptical morphology, with a high degree of central concentration. There is minimal evidence of distinct spiral arms or a prominent disk structure. The overall color appears yellowish-orange, suggestive of an older stellar population dominated by evolved stars. There are no readily apparent signs of significant ongoing star formation, such as bright blue regions associated with young, massive stars. The galaxy appears largely undisturbed, with no obvious signs of major mergers or significant tidal interactions. A faint, diffuse halo may be present, extending slightly beyond the main body of the galaxy. The shape is generally round, with only a slight elongation. It appears to be a fairly massive galaxy, likely a lenticular or elliptical type.
