The galaxy presents a somewhat smooth, elongated morphology. The dominant feature is a central bulge that appears yellowish-orange, suggesting an older stellar population with relatively low ongoing star formation. Extending outwards from the bulge, a faint, diffuse disk is visible. The disk appears bluer in hue relative to the bulge, implying the presence of younger, hotter stars and regions of recent star formation. The galaxy lacks any obvious spiral arm structure or prominent dust lanes, and no strong tidal features or signs of a major merger are visible. There may be a minor perturbation of some kind, but nothing significant. The general impression is that of a galaxy with a well-established structure that is not presently undergoing major disruptive events.
