The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with a high degree of roundness. A prominent bulge is visible, exhibiting a bright yellowish-white core that gradually fades into a less defined outer region. There is little evidence of spiral arm structures or significant dust lanes. The color profile suggests a population dominated by older stars, with a weak indication of ongoing star formation. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal interactions. The galaxy is likely a massive one, with a detectable rate of star formation.
