The galaxy appears to be a somewhat compact object, with a concentrated core region. The overall shape is difficult to discern definitively, but a slight elongation or flattening is suggested. The light distribution indicates a smoother profile, transitioning from a brighter central region to a fainter, less defined outer halo. There is no clear evidence of spiral arms or a distinct disk structure. There is a subtle patch on the right side of the galaxy, perhaps indicative of merging or tidal interactions. The dominant color appears to be bluish, which could be indicative of a younger stellar population or ongoing star formation. Overall, this galaxy presents a morphology potentially consistent with an elliptical or lenticular galaxy, though the possibility of it being a spiral viewed at an angle cannot be ruled out without further data.
