The galaxy presents as a moderately inclined, possibly late-type spiral or an irregular disc galaxy, though at this resolution distinguishing between the two is difficult. It exhibits a somewhat elongated morphology, appearing roughly cigar-shaped. The central region displays a brighter, more condensed light profile, suggestive of a bulge, but it is not particularly pronounced. The outer regions of the galaxy become more diffuse, hinting at the presence of a disk structure, though distinct spiral arms are not clearly visible in this image. The galaxy appears blueish in color, indicating a likely presence of young, hot stars and ongoing star formation, though the specific distribution of star forming regions cannot be resolved. There is no obvious evidence of a major merger event, tidal tails, or other strong gravitational disturbances, though subtle asymmetries cannot be ruled out at this scale.
