The galaxy presents as a somewhat elliptical, though not perfectly round, form. The light profile appears relatively smooth, with a concentrated central bulge. Faint extensions are barely perceptible but seem uniform, suggestive of a fairly quiescent state. Color gradients indicate a possible radial change in stellar population, with a bluer core and redder outer regions. This hints at ongoing star formation concentrated in the central region, alongside an older stellar population dominating the outer regions. There is no sign of strong spiral arm structure, a bar, or any major tidal disturbances. A slight elongation is apparent, indicating it is not perfectly spherical. Based on the light distribution, this galaxy appears to be an early-type spiral or elliptical galaxy with some degree of recent or ongoing central star formation.
