The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests a dominant population of older stars, exhibiting a yellowish to reddish hue, particularly concentrated towards the galactic center. The central bulge is prominent and appears to be the brightest region. There is a faint, diffuse disk extending outwards from the bulge, though the arms are not well-defined or tightly wound. Little to no evidence of active star formation is apparent, as indicated by the lack of strong blue color components. There's a possibility of minor tidal disturbances or interactions based on subtle asymmetries.
