The galaxy presents as a centrally concentrated elliptical system. The light profile exhibits a smooth, diffuse character with a gradual decline in surface brightness from the core outwards. There is a hint of a slightly elongated shape, deviating from perfect circularity. A prominent bulge dominates the structure, with a relatively small, faint disk. The overall color of the galaxy leans towards the red end of the spectrum, indicative of an older stellar population with relatively low levels of ongoing star formation. There is no distinct evidence of spiral arm structures or prominent dust lanes. No significant tidal features or signs of recent merger activity are immediately apparent, although minor disturbances cannot be ruled out. 
