The galaxy appears to be a relatively luminous object, likely a spiral, exhibiting a fairly concentrated bulge and a disk component that is somewhat diffuse, with an apparent diameter of approximately 6.6 kpc. There is an indication of spiral arm structure, but the resolution limits a detailed assessment. The galaxy displays a yellow-reddish hue, suggesting a significant population of older stars, or a considerable amount of dust obscuring bluer, younger stars. There is a likelihood of ongoing or recent merger activity, suggested by the galaxy's amorphous appearance and an extended tidal-like feature on one side. This merger may be contributing to the formation of new stars, but this is difficult to discern from the image alone. The galaxy is moderately massive and exhibits an estimated amount of star formation. Overall, the observed characteristics suggest an intermediate to late-stage galaxy that is actively interacting and/or undergoing morphological transformation.
