The galaxy presents a generally smooth morphology, with a centrally concentrated luminosity profile suggesting a dominant bulge component. The overall shape approximates an elliptical form, with a slight deviation from perfect roundness. The color profile exhibits a redder hue, indicative of an older stellar population and a reduced rate of on-going star formation. There are no obvious signs of spiral arm structures or significant dust lanes. Minor disturbances are possibly present. The light is concentrated in the center, suggesting it is likely a spheroidal galaxy with limited recent interaction.
