This galaxy presents as a relatively smooth, amorphous structure. It appears to be somewhat elliptical in shape, though not strongly so. The central region exhibits a brighter, more concentrated glow, suggesting the presence of a core or nucleus. A faint disk component may be present but is difficult to resolve with certainty. There are indications of some structural disturbances with a possibility of tidal interactions or minor merging event, evident in the asymmetry and faint extensions of the galaxy's outer regions. In general, the galaxy appears relatively quiescent, with limited evidence of active star formation in this image, but also with subtle hints of recent activity.
