The galaxy presents as a relatively compact object. Its morphology appears largely smooth and elliptical, exhibiting a high degree of central concentration. There is little evidence of spiral arm structure or significant disk features visible in this observation. The galaxy's color index suggests a dominant population of older stars, appearing reddish in overall color. Faint color variations within the galaxy may imply some ongoing, albeit low, level of star formation. There are no obvious signs of major mergers or significant tidal disturbances in this image. Faint asymmetric light could suggest a past minor interaction. Based on its size and apparent magnitude, this galaxy appears to be a moderately sized system at a considerable distance.
