The galaxy appears as an elliptical or lenticular type. It exhibits a smooth, relatively featureless morphology, lacking prominent spiral arms or a distinct disk structure. The core of the galaxy displays a high degree of central concentration, with light intensity decreasing gradually towards the outer regions. The shape is mostly in between, but closer to round with no strong elongation or distortion visible. There is no evidence of ongoing major mergers or significant tidal disturbances in this image. The galaxy is relatively large, implying a significant stellar mass. The color indices suggest that the galaxy is comprised of mostly older stars, indicating a relatively low current star formation rate.