The object presents as a galaxy, likely a spiral, observed nearly edge-on from our vantage point. A prominent, dusty disk is visible, obscuring the central bulge. The disk appears reddish-orange, indicative of an older stellar population and dust absorption. The bulge shows a smooth, concentrated light distribution and a slight boxy appearance. There appears to be little evidence of significant recent merger activity or tidal disturbances. The apparent size suggests a moderately sized galaxy. Based on the colors, the star formation rate is likely low. 
