The galaxy presents as a relatively smooth, disk-like structure, exhibiting a shape somewhere between round and elongated. There's a central, brighter bulge region that appears somewhat concentrated, surrounded by a less luminous and more diffuse disk. There is little evidence of prominent spiral arm structure. The color distribution suggests an older stellar population dominating the galaxy's light, appearing to be yellowish-red in the central regions and slightly bluer in the outer parts of the disk. There may be minor tidal disturbances in the galaxy's morphology. Based on these observations, this galaxy might be classified as an intermediate-type spiral, with a relatively low rate of star formation.
