The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution. There are no prominent spiral arms visible, and the overall structure appears featureless, suggesting an older stellar population. The galaxy shows a mild elongation, appearing slightly cigar-shaped. A concentration of redder light is observed towards the center, potentially indicative of a higher density of older, redder stars within the galactic nucleus. There is a faint bluish halo surrounding the central region, which may indicate the presence of some younger stars. No significant signs of ongoing mergers or major disturbances are evident in its overall morphology. The estimated mass range and star formation rate suggest that it is a large galaxy with low star forming properties.
