The galaxy presents an elongated morphology, appearing somewhat cigar-shaped. It appears to be a relatively large galaxy, potentially around 7 kpc in radius. The light distribution seems smooth, lacking prominent spiral arm structures or a bright, concentrated nucleus.  There's a hint of blueish light in parts of the galaxy, which could indicate regions of on-going star formation, but the majority of the galaxy appears redder in color, which could be suggestive of an older stellar population and a lower star formation rate. There may be some minor disturbances or irregularities in its shape, but it does not appear to be undergoing a major merger.
