The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is roughly elliptical, appearing neither perfectly spherical nor highly elongated. The core exhibits a bright, diffuse glow that fades gradually towards the outer edges. No distinct spiral arm structures or prominent dust lanes are discernible. The colour profile suggests a population of older stars, displaying a yellowish hue, with hints of redder components closer to the nucleus. There is little evidence of active star formation, with the overall texture being fairly uniform and devoid of bright, blue knots associated with young stellar clusters. There appears to be no signs of any major ongoing merger activity or tidal disturbances.
