The galaxy presents as a generally smooth object. The central region appears to be a bright, concentrated spheroid, indicative of a substantial bulge component. Moving outward from the core, the light diffuses and fades relatively quickly, suggesting a lack of extended disk structure. The galaxy’s overall shape is largely circular, deviating little from a perfect ellipse. There are subtle irregularities in the outer halo, hinting at the possibility of minor tidal disturbances or ongoing accretion events, although no clear signs of a major merger are observed. The colour profile reveals a significant red component to the light, increasing towards the central bulge, suggesting an older stellar population dominates, with a reduced rate of recent star formation throughout the galaxy.
