The galaxy appears to be a spiral galaxy, observed at a slight angle. It is characterized by a prominent central bulge exhibiting a yellowish hue, indicative of an older stellar population. Two spiral arms emerge from the bulge, one considerably more defined than the other. The spiral arms display a winding morphology between medium and tight, as well as evidence of active star formation regions, suggested by the blue-ish tint observed in the spiral arms. Overall, the galaxy appears to be fairly isolated. There is a clear lack of evidence of tidal disturbances or a major merger. However, the galaxy's asymmetrical shape, the ill defined arms, and areas of brightness on the outer edges suggest it may be undergoing a minor merging event or has undergone a merging event in the relatively recent past. The core is surrounded by areas of low star formation.
