The galaxy appears as a relatively bright object with an approximate effective radius of 7.8 kpc. The galaxy demonstrates a smooth morphology with a central concentration of light. A slight disk is visible as the edge on green band, but overall there are little prominent features in the galaxy's structure. There is a possible sign of minor interaction, but the object seems to be primarily isolated, not undergoing any major merging activity. The colors indicate the galaxy contains a substantial population of relatively older stars, and the estimated magnitude indicates it is luminous.
