The galaxy appears to be a relatively compact object with a smooth overall structure. The galaxy does not display a strong spiral arm structure, nor does it appear perfectly elliptical; however, there is a faint hint of a disk-like structure. There are no prominent features such as strong dust lanes or a bright, actively star-forming nucleus that can be discerned in the available image. There are indications of minor disturbances within the galaxy, evidenced by the galaxy's irregular shape. There are no clear signs of interaction with other galaxies, although the faintness of the image makes it difficult to completely rule out tidal distortions or other merger-related features. The object exhibits a general color profile that is redder than what would be expected from a very actively star-forming galaxy, suggesting that it may be dominated by an older stellar population. There are suggestions of star formation activity, though, as there are localized bluer regions within the overall redder structure.
