The galaxy appears as a moderately inclined, disk-shaped system. There is a prominent central bulge that exhibits a yellowish hue, suggesting an older stellar population dominating this region. Emanating from the central bulge is a faint disk structure, tinged with bluish colors, suggestive of ongoing star formation. The disk is not perfectly smooth, showing some subtle irregularities and possible spiral arm segments. There appears to be a slight asymmetry or warp in the disk structure. The galaxy displays no obvious signs of a major merger event, though minor tidal disturbances may be present. The overall morphology leans towards a late-type spiral, exhibiting characteristics transitional between a smooth elliptical and a well-defined spiral structure. The galaxy is of intermediate size.
