The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a centrally concentrated luminosity profile that decreases gradually outwards. The core region presents a bright, yellowish hue, suggesting an older stellar population with a lack of significant recent star formation. There is a slight elongation to the galaxy's shape, leaning towards a somewhat rounded, yet not perfectly spherical, morphology. No distinct spiral arms, dust lanes, or other prominent features typically associated with spiral galaxies are readily apparent. There is no clear evidence of any major ongoing mergers or significant tidal disturbances affecting the system's overall structure, although there might be minor irregularities that could imply past interactions or minor disturbances. The galaxy appears relatively isolated in this field.
