The galaxy presents as a spiral type, although the disk inclination is relatively face-on, limiting detailed observation of its structure. There is a moderately sized central bulge that graduates into a disk. Spiral arms are visible. The galaxy exhibits a range of colors, with a redder hue concentrated in the central bulge region, suggesting an older stellar population, potentially indicating a lack of active star formation in this region. The outer disk appears bluer, indicative of younger, hotter stars and ongoing star formation. No significant signs of tidal disturbances or interactions with other galaxies are immediately apparent. The galaxy has a low-moderate redshift value. The estimated size of the galaxy is a few kiloparsecs.
