The galaxy appears to be a relatively smooth, elongated object, presenting an edge-on or highly inclined disk morphology. The light distribution seems fairly uniform, with a brighter central region suggesting a bulge. There is little evidence of spiral arm structure or distinct star-forming regions within the visible light. The overall color is consistent with an older stellar population, with a possible slight blue tint from any newer stars that are forming. The galaxy appears to be undisturbed, with no signs of major mergers or significant tidal interactions. The elongated shape of the galaxy, combined with its smooth appearance, suggests it could be an edge-on spiral galaxy or potentially a lenticular galaxy.
