The galaxy presents as a late-type spiral, likely viewed at a moderate inclination. A distinct disk structure is observable, characterized by a brighter central bulge region that fades gradually towards the outer edges. The spiral arms are not clearly defined, suggesting a flocculent spiral structure. Some irregular, fainter regions are present in the disk, possibly indicating areas of ongoing star formation. The galaxy exhibits an overall redder color, particularly within the central bulge region, suggesting an older stellar population. The disk appears slightly bluer, potentially indicating the presence of younger stars and active star forming regions. There appears to be a very slight asymmetry in the shape of the galaxy's disk, potentially indicating a recent minor interaction.
