The galaxy presents as a relatively smooth, centrally concentrated structure. It appears largely spheroidal, with a high degree of circularity and no obvious spiral arm features. The color profile suggests a predominantly older stellar population, exhibiting a yellowish-red hue, with a touch of bluer light in the outer regions. There's no immediately visible evidence of significant ongoing star formation, though subtle variations in color may indicate some low level activity. There is no sign of any major disturbance to the primary galaxy structure, such as tidal tails or shells, however there is the possibility of a minor merger.
