The galaxy presents as a relatively smooth, elliptical-like object with a notable central bulge. It displays a diffuse, even light distribution with a lack of clearly defined spiral arm structures. There appears to be a slight elongation. The galaxy exhibits a color profile suggesting an older stellar population, with a greater proportion of redder wavelengths, and minimal evidence of active star formation. There may be a hint of minor tidal disturbance, though the object is largely undisturbed. The light profile seems centrally concentrated, with gradually decreasing intensity outwards towards the faint edges of the galaxy.
