The galaxy presents a generally smooth, elliptical morphology, though subtle irregularities suggest the possibility of minor disturbances. The light distribution appears centrally concentrated, exhibiting a bright, yellowish core that gradually diffuses outwards. The overall shape is largely round, with a slight elongation. Faint bluish hues are visible in the outer regions, suggesting the presence of some younger stars or ongoing star formation, albeit at a relatively low rate. There is no clear evidence of spiral arms or a well-defined disk structure. Based on the light profile and overall appearance, this galaxy likely represents a relatively massive system, currently experiencing low levels of star formation. There is no obvious sign of interactions with any other system.
