The galaxy presents as a relatively smooth, elliptical structure. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population dominated by evolved stars. Moving outward from the core, the light gradually diminishes. A faint, redder halo extends beyond the central region, exhibiting a less structured appearance. There is no visible evidence of spiral arms or significant dust lanes. The overall morphology appears undisturbed, without any obvious signs of recent merger activity or tidal interactions. It seems to be a fairly massive system with a moderate amount of star formation.
