The galaxy presents as a diffuse, elliptical object with a bright, concentrated core. The morphology appears generally smooth, with a noticeable lack of distinct spiral arm structures or prominent dust lanes. The color profile indicates a slightly yellowish hue, suggesting an older stellar population. There is a hint of a less luminous halo extending beyond the central region, but its boundaries are poorly defined. Overall, the galaxy seems to be relatively undisturbed, without strong evidence of recent merger activity or significant tidal interactions. The general form and color suggest a relatively quiescent state, with a low rate of ongoing star formation.
