The galaxy presents as a moderately inclined disk galaxy. Its morphology is relatively smooth, appearing elliptical in shape without prominent spiral arms. The central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. Progressing outwards from the bulge, the disk appears bluer, which is indicative of more recent star formation within its spiral structure. The light distribution across the disk is fairly even, though there are some areas of faint asymmetry. The overall color profile suggests ongoing star formation. The galaxy appears relatively isolated with no obvious signs of recent tidal interactions or mergers.
