The galaxy presents as a relatively compact, disk-shaped structure, viewed at a shallow angle to our line of sight. The central bulge is prominent and exhibits a smooth, bright appearance, suggesting an older stellar population. The disk appears to be relatively smooth and uniform, with only faint traces of spiral arm structure visible, particularly on the near side. There is a suggestion of a tidal disturbance or interaction on the left side. This disturbance displays a bluer hue than the main body of the galaxy, possibly indicating a region of active star formation triggered by the interaction. Overall, the galaxy appears to be in a state of minor interaction or disturbance, with evidence of ongoing, albeit perhaps low-level, star formation. The galaxy appears to have a modest mass.
