The galaxy presents as an elongated, cigar-shaped structure. The light distribution suggests a central bulge that graduates into a disk with diffuse boundaries. The overall color appears reddish, indicating a likely older stellar population. The structure appears relatively smooth with some suggestion of a possible minor disturbance or interaction, as the light appears slightly irregular and asymmetrical. The galaxy shows a substantial red shift, likely far away. The physical size of the galaxy is approximately 9 kpc based on the Petrosian radius measurement, suggesting a moderately sized galaxy. The inferred star formation rate of the galaxy is relatively low, likely due to a population of older stars.
