The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears largely uniform, diminishing gradually from the core outwards. There is minimal evidence of spiral arms or pronounced dust lanes. The color profile suggests an older stellar population, with a general lack of intense blue regions indicative of recent star formation, though there appears to be a faint, bluer halo surrounding a more central concentration of yellow-white light. Overall, the galaxy appears to be a relatively undisturbed system, exhibiting a lack of significant tidal features or ongoing mergers, and is close to being circular in shape.
