The galaxy appears to be an elongated, cigar-shaped system. Its light profile is dominated by redder wavelengths, indicating an older stellar population. There may be a disk galaxy undergoing a minor interaction. There is some evidence of disruption in the light distribution, but without high resolution data it is difficult to determine the precise nature of this feature. Overall, the galaxy presents as relatively smooth, with no readily apparent strong spiral arm structure or prominent dust lanes visible in this imaging.
