The galaxy presents a predominantly smooth morphology, with little evidence of spiral arms or a distinct disk structure. The light distribution appears relatively concentrated, suggesting an elliptical or lenticular classification. The color gradient indicates a central concentration of older stellar populations, exhibiting a reddish-yellow hue. There are slight color variations in the galaxy, with a faint blue tinge possibly indicating areas of more recent star formation. The galaxy's shape is generally round. There is no significant evidence of tidal features or ongoing major merger activity, although there appears to be some minor disturbance or asymmetry in the outer regions, suggesting a potential interaction.
