The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, concentrated light profile. It possesses a distinct central bulge, gradually fading into a fainter, extended halo. There is a subtle color gradient visible, transitioning from a yellowish hue in the core to a slightly redder tint towards the outer regions. No prominent spiral arms or dust lanes are discernible. The galaxy exhibits a round shape, with no major disturbances or signs of ongoing mergers visible in this image. The overall morphology suggests an older stellar population, with a relatively low star formation rate.
