The galaxy presents as an elliptical type, exhibiting a smooth, concentrated central bulge that dominates the overall luminosity. The light distribution appears fairly even, with no strong evidence of spiral arms or significant dust lanes. There is a slight elongation to the galaxy's shape, indicating a non-spherical structure. The color profile suggests an older stellar population, indicated by the yellowish hue, particularly concentrated towards the core, which suggests a paucity of ongoing star formation within the central region. A faint blue halo surrounds the central body, indicative of a younger stellar population, but it is largely overwhelmed by the yellow core, indicating older stars. Overall, the galaxy is a relatively symmetrical elliptical with a dominant bulge and little evidence of active star formation.
