The galaxy presents a generally smooth morphology. It appears elliptical, with a nearly circular shape. The color profile suggests a population of older stars, with a yellowish hue dominating the central region. There's a subtle color gradient, shifting towards redder tones in the outer regions of the galactic halo. No distinct spiral arms, bar structures, or signs of recent major mergers are readily apparent. Minor irregularities or disturbances may be present, but they are subtle and do not significantly disrupt the overall smooth profile. Star formation rate appears to be relatively low, consistent with an older stellar population.
