The galaxy presents as a generally smooth, centrally concentrated object. The morphology suggests a predominantly elliptical shape, with a high degree of roundness. The light distribution appears relatively uniform across the galaxy, with a subtle color gradient apparent with a slightly bluer core, possibly indicating a younger stellar population. The isophotes are regular and there are no distinct tidal features or prominent dust lanes visible in this image that would suggest a recent major merger event. There may be minor disturbances present, but are not readily visible in the image. Based on the data, this galaxy has an estimated mass of 10^9.3 solar masses, suggesting a relatively low-mass system. Overall, the characteristics point to a spheroid-dominated galaxy with minimal ongoing star formation.
