The galaxy appears to be a spiral galaxy viewed at a slight angle. It displays a bright, concentrated central bulge that graduates into a more diffuse disk.  A faint, blue-ish spiral arm structure can be tentatively identified on opposing sides of the center, suggesting ongoing star formation in these regions.  There is some subtle disruption apparent in the outer regions. The disk component exhibits a color gradient, with the innermost regions showing yellow-ish hues indicative of an older stellar population.