The galaxy presents as a somewhat elliptical, likely disc galaxy, seen at an intermediate angle. The central bulge appears bright and concentrated, exhibiting a yellowish hue, which may suggest an older stellar population. Surrounding the bulge is a less concentrated, bluer region of what are presumably spiral arms and an accompanying disc, but the arms are not very well defined. The overall structure appears largely undisturbed, though there may be some minor irregularities in the outer regions of the disc, suggesting potential interactions or tidal effects. The galaxy's color suggests ongoing star formation within the spiral arms, but with a larger proportion of older stars in the central bulge.
