The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution appears fairly uniform, with a bright, somewhat diffuse core that gradually fades towards the outer edges. There are no obvious spiral arm structures or distinct features indicative of active star formation regions. A slight color gradient is observable; the core exhibits a yellowish hue, suggesting an older stellar population, while the outer regions appear slightly redder. There is no strong evidence of recent or ongoing mergers or tidal disturbances impacting the galaxy's overall structure. The overall impression is that of an evolved galaxy, likely an elliptical or lenticular type, with a significant fraction of its stellar mass already formed.