This galaxy presents as an edge-on spiral. A prominent, moderately bright central bulge is apparent, exhibiting a slightly reddish hue indicative of an older stellar population. The disk appears thin and elongated, displaying a faint bluish tint especially towards the outer edges, suggestive of more recent star formation in these regions. The lack of distinct spiral arm structure indicates the disk is relatively smooth. There is no apparent evidence of any major mergers or significant tidal disturbances. The galaxy seems relatively isolated, maintaining a stable, non-interacting state.
