The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. Its overall form lacks any prominent spiral arms or distinct features, suggesting it may be an early-type galaxy. The color profile appears generally uniform, with a slight tendency towards redder hues, implying a stellar population dominated by older, redder stars and limited recent star formation. There is no visible indication of ongoing major merger events, although subtle disturbances cannot be ruled out. The galaxy's shape is neither perfectly spherical nor highly elongated, tending more toward an intermediate elliptical form.
