The galaxy presents as a relatively smooth, single structure. There is a dominant central bulge, with a yellowish hue indicating an older stellar population. Surrounding the bulge is a fainter disk which appears featureless. There is no evidence of spiral arm structure or significant dust lanes. The disk component shows a slightly bluer color than the central bulge, suggestive of ongoing, albeit low-level, star formation. The galaxy appears more rounded in shape, but not perfectly circular. There is a suggestion of minor tidal disturbance or interaction, potentially a slight asymmetry in the outer regions of the disk, but it is difficult to determine the origin of this disturbance. There are no distinct features of a merging event visible.
