This galaxy presents as a smooth, centrally concentrated object, displaying characteristics of an elliptical galaxy, or possibly a lenticular galaxy viewed at a slight angle. The light distribution exhibits a relatively high degree of symmetry, with a smooth transition in surface brightness from the core outwards. The central region appears yellowish-white, suggesting an older stellar population dominates the core, with fewer young, massive stars contributing to the overall luminosity. The outer regions appear to fade to a more reddish hue, potentially indicating a population of even older, redder stars in the galaxy's halo or disk. There's a very slight hint of a possible flattened disk-like structure, though the dominant impression is that of a spheroid. No distinct spiral arms or prominent dust lanes are visible. There is no obvious evidence of a recent major merger event, although there are some subtle irregularities in the outer isophotes that could be indicative of minor past interactions. 
