The galaxy presents as an elliptical or lenticular structure, exhibiting a relatively smooth light distribution. The primary body of the galaxy appears elongated, with a ratio of major to minor axes indicating a moderate ellipticity. The core region displays a somewhat concentrated brightness. A slight color gradient is observed, with the central region exhibiting a bluer hue, possibly indicative of younger stellar populations or ongoing star formation, although at a low rate. The outer regions appear redder, suggesting older stellar populations. The overall structure lacks prominent spiral arms or a well-defined disk. There is a hint of some disturbance in the upper right corner of the image which may be an artifact, or a tidal tail. The galaxy does not appear to be undergoing any major merging events, although there may be a minor interaction occurring.
