The galaxy presents as an edge-on spiral or lenticular galaxy. The disk is clearly visible as a linear structure, obscuring a concentrated central bulge. The bulge appears to be round, with a smooth profile. There is no evidence of spiral arm structure discernible within the disk at this resolution. The galaxy's color suggests a population of older stars with a limited amount of on-going star formation. There are no signs of any major mergers or tidal disturbances. It appears to be a relatively undisturbed system. The mass is estimated to be between 10^8 and 10^9 solar masses. The specific star formation rate is low, indicating the galaxy is likely to be approaching the red sequence. The galaxy shows little or no signs of recent interaction.
