The object presents as a spiral galaxy with a redshift value suggesting a relatively nearby location. The galaxy appears to be moderately inclined to our line of sight. A prominent central bulge, appearing a yellowish-orange hue, dominates the central region. Faint spiral arms extend outwards from the central bulge, exhibiting a tightly wound morphology. Evidence of ongoing star formation, characterized by bluer hues, is visible within the spiral arms, though the overall star formation rate appears to be subdued. The galaxy appears relatively isolated with no obvious signs of significant tidal interaction or merging activity, although some minor disturbances cannot be ruled out. A faint bar-like feature may be present across the central region. Overall, the galaxy presents as a mature spiral with characteristics of a disk galaxy.
