The galaxy presents as a somewhat smooth, luminous structure, possibly elliptical in morphology, displaying a concentrated central bulge that fades into a more diffuse halo. There may be some distortions or minor disturbances visible in the outer regions, potentially indicating past or ongoing gravitational interactions. The colour profile reveals a general reddening of the stellar population, suggesting an older stellar age and low ongoing star formation, however, there appears to be some blue coloration on the top of the galaxy indicating areas of possible active star formation. Its overall shape can be characterized as moderately rounded, leaning towards an intermediate state rather than perfectly circular or elongated.
