The galaxy appears as a centrally concentrated, elliptical-like object. Its light profile is smooth, lacking prominent spiral arms or distinct features indicative of active star formation. The central region exhibits a high surface brightness, gradually decreasing towards the outer edges, suggesting a relatively uniform stellar population distribution. The shape is more in-between than perfectly round, but closer to round than cigar-shaped. There's no immediately apparent visual evidence of any ongoing merger activity or significant tidal disturbances affecting its structure. The galaxy displays a color gradient, being relatively redder in its core and becoming slightly bluer towards the edges. This could indicate a mixed stellar population, with older, redder stars concentrated in the center and younger, bluer stars in the outskirts, though the difference is subtle.
