The galaxy presents a generally smooth morphology, with a moderately elongated, cigar-like shape. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. A subtle blueish tint is visible in the surrounding area, which may indicate regions of more recent, but relatively weak, star formation. There is no clear spiral arm structure, though some disk-like features may exist. Some potential minor gravitational disturbances seem to be present. Overall, this galaxy appears to be a relatively massive system, with an intermediate star formation rate.
