The galaxy presents a largely smooth morphology, with a concentrated central bulge dominating its appearance. The light distribution appears relatively even and symmetric, suggesting a lack of significant spiral arm structure or irregular features. There is a slight elongation, deviating from a perfectly circular shape. The central region exhibits a bright, yellowish hue, transitioning to a redder tone towards the outer edges of the galaxy. There is no evidence of ongoing major merging activity, but the galaxy is not perfectly spherical, indicating that minor disturbances may have occurred. The galaxy appears to be a relatively massive, evolved system with a low rate of star formation.
