The galaxy presents as a somewhat elongated structure. The light distribution appears uneven, with a brighter, more concentrated region displaying a yellowish hue at one end. This could indicate an older stellar population, perhaps a bulge component.

A fainter, bluer area is observed towards the opposite end of the galaxy, possibly indicative of ongoing or recent star formation. This area might be a star-forming region or a spiral arm segment. There is a suggestion of tidal interaction or perhaps a past merger event, given the asymmetry and disturbed appearance. Overall, the galaxy appears to be undergoing some form of dynamic evolution.
