The galaxy appears as a centrally concentrated, ellipsoidal structure. The core exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. There is little evidence of spiral arms or significant disk features; the overall light distribution seems smooth. The galaxy's color profile indicates a dominance of older stars in the nucleus with a lack of significant blue, recently-formed stars. There is a subtle falloff in light intensity from the core towards the outer regions of the galaxy, with no prominent tidal features or signs of major disturbances. The galaxy presents a compact appearance, displaying an overall regularity in shape.
