The galaxy appears to be a disk galaxy, although the disk is relatively faint. It is likely seen at a slight inclination. The central bulge is bright and yellowish, suggesting an older stellar population. There are very faint blue arms/regions that may indicate active star formation. The overall color is redder than average, suggestive of a significant population of older stars and possibly a lower rate of ongoing star formation. The shape appears to be more elliptical than circular, likely due to being seen at an angle. There are no signs of any recent major merger events; however, the light distribution in the outer regions is uneven, with a slight amount of faint fuzz, and thus there may have been a minor interaction.
