This galaxy appears to be a relatively face-on system, exhibiting a primarily smooth morphology. The light is concentrated towards the center, suggesting a prominent bulge. The overall shape is elliptical, leaning towards round, without any obvious strong distortions or tidal features suggesting a major merger, though there is some evidence of minor disturbances within the outer disk. Color gradients suggest a redder central region potentially dominated by older stellar populations, with a bluer hue extending into the surrounding disk where younger stars may reside. The galaxy exhibits characteristics of a relatively massive system, with an estimated size of approximately 6 kpc across its half-light radius. Star formation activity appears to be relatively low within the galaxy.
