The galaxy presents an elliptical morphology, with a high degree of central concentration. A luminous, yellowish core region dominates, suggesting a significant population of older stars. The overall light distribution appears smooth. There may be a faint, bluer disk component evident, contributing to a slight flattening along the major axis. There is no clear evidence of spiral arms, bar structure, or distinct dust lanes. Minimal signs of recent major merger activity or significant tidal disturbances are apparent, although subtle asymmetry may indicate a past minor interaction. The galaxy exhibits a substantial stellar mass and moderate star formation activity.