The galaxy appears as a concentrated, centrally brightened object with a generally smooth morphology. Its light distribution suggests a spheroid-dominated system, exhibiting a roughly elliptical shape that tends toward round. There is little discernible evidence of spiral arm structures or significant dust lanes within the disk. The galaxy's color profile indicates a population of older stars. There is a suggestion of a low level of recent star formation activity, but this does not visibly impact the overall color profile.
