The galaxy presents as a face-on or slightly inclined spiral, approximately 2.5 kpc in diameter, as estimated from petrosian radius. A central bulge appears subdued or nonexistent, with luminosity distributed relatively evenly throughout the disk. Spiral arm structure is discernible but somewhat flocculent; regions of active star formation are suggested by blue-ish color. Overall, the light profile is somewhat irregular, hinting at ongoing interaction or merging activity with a possible minor companion. There is a very faint hint of a bar. Based on the distributed light and apparent lack of a distinct, bright bulge, the galaxy is likely a late-type spiral.
