The galaxy presents a predominantly smooth morphology, appearing as an elliptical galaxy rather than a spiral. Its shape is neither perfectly round nor elongated, leaning more towards an intermediate elliptical classification. There is no apparent disk structure. Color gradients indicate a higher concentration of older stellar populations within the central bulge, exhibiting a yellowish hue, with some redder areas. There is no evidence of any on-going major merger events or significant tidal disturbances in the image, though there may be a faint small disturbance in the image. No distinct dust lanes or prominent star-forming regions are visible, suggesting a relatively low star formation rate.
