The galaxy presents as a spiral type, observed at a moderate inclination. Its morphology suggests the presence of well-defined spiral arms extending from a central bulge. The arms exhibit a relatively medium winding pattern. The bulge appears moderately sized compared to the disk. The galaxy's color profile indicates ongoing star formation, particularly within the spiral arms, as evidenced by the bluer hues. The presence of some yellow and red near the bulge suggests the existence of an older stellar population. There is some evidence of potential tidal distortion or interaction with another galactic object, though more data is required to confirm this hypothesis. Overall, the galaxy exhibits characteristics consistent with a late-type spiral galaxy undergoing active star formation.
