The galaxy presents an elliptical morphology, exhibiting a central bulge that appears bright and concentrated. The isophotes are generally smooth, suggesting a relatively relaxed stellar distribution. The galaxy displays a color gradient, with the core appearing bluer and transitioning to a redder hue towards the outer regions. There is some indication of subtle disturbances in the form of faint tidal features or asymmetric light distribution, potentially indicating a past or ongoing minor interaction with another galaxy. However, these features are not overtly prominent. Overall, it appears to be a relatively quiescent galaxy, though further spectroscopic analysis would be needed to determine its precise composition and internal dynamics.
