The galaxy presents as a generally smooth, elliptical morphology. Its light profile is centrally concentrated, with a gradual decrease in intensity outward from the core. The color appears relatively uniform across the galaxy, with a slightly yellowish hue, suggesting an older stellar population dominating the light output. There is no clear evidence of spiral arms, a distinct disk, or ongoing major mergers. Faint, subtle irregularities can be observed in its outer regions, which may indicate a minor interaction or accretion event in the past. The galaxy appears to be relatively isolated, without any obvious, significant companion galaxies in close proximity. The overall structure is compact and symmetrical, which indicates it could be a highly relaxed system.
