The galaxy presents as a centrally concentrated object, exhibiting a somewhat smooth appearance overall. The light distribution appears relatively uniform with no obvious spiral arm structures or a prominent bulge. The morphology is suggestive of a disk galaxy, however, the structure is quite hazy, and the lack of sharp features suggests the light is largely coming from an older stellar population. The overall color of the galaxy leans towards the redder end of the spectrum. This reddish hue might be indicative of an older stellar population. There is a slight asymmetry in the light distribution, implying a possible minor disturbance of some sort.