The galaxy presents as an elliptical-type system, exhibiting a largely smooth and featureless morphology. The central region displays a concentrated, yellowish hue, suggesting a population of older stars. A gradual color gradient is observed outward from the core, transitioning to a slightly bluer periphery, indicative of a younger stellar population or ongoing star formation, although this activity appears limited. The galaxy appears generally rounded in shape, with only a slight elongation. No prominent spiral arms, dust lanes, or significant tidal disturbances are evident. The overall structure suggests a relatively relaxed system with limited recent merger activity.
