The galaxy presents as a relatively small, edge-on spiral system. A central bulge is clearly visible, appearing bright and somewhat diffused, hinting at an older stellar population. The disk is well-defined and extends significantly beyond the bulge. It shows a blueish hue, possibly indicating ongoing star formation, particularly in the outer regions. There appears to be some evidence of dust lanes obscuring parts of the disk, though the resolution limits detailed analysis. Overall the system appears relatively undisturbed, showing no strong evidence of a major merger or tidal interactions, although minor disturbances cannot be ruled out.
