The galaxy presents as a somewhat elongated, disk-like structure viewed at an oblique angle, showing characteristics of a spiral galaxy. The central bulge exhibits a brighter, yellowish hue, suggestive of an older stellar population. Fainter blueish regions are distributed within the outer portions of the disk, possibly indicating areas of more recent or ongoing star formation. There appears to be a faint hint of spiral arm structure, though the resolution limits detailed characterization. No strong signs of tidal disruption or major merger events are immediately apparent, though some minor irregularities in the disk's shape are not ruled out. The overall color suggests the galaxy lies within the "green valley" region on the color-magnitude diagram, between primarily star-forming and quiescent populations.
