The galaxy appears as a somewhat diffuse object, exhibiting a largely smooth morphology. There is a central, brighter region with a more concentrated light profile, possibly indicating a bulge.  The overall shape approximates a rounded structure. An extension of fainter material is observed extending from the main body, possibly suggestive of tidal interactions or minor disturbances to the galaxy's structure. There is minimal evidence of spiral arms or strong dust lanes, but a slight color gradient suggests some internal structure. The overall color profile implies an older stellar population, with a likely low star formation rate. A possible merger or tidal interaction is suggested by its irregular shape.
