The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, bright central bulge that transitions gradually into a fainter, more diffuse halo. The overall shape is predominantly round with a slight elongation suggesting it may be more of an oblate spheroid. No distinct spiral arms or bar structures are discernible. There is no apparent major merging activity or tidal features. The color profile suggests an older stellar population, especially within the bulge, with a shift towards redder wavelengths. There appears to be little evidence of active star formation, given the lack of blue emission. Minor disturbances can be observed in the form of slight asymmetry in the outer regions of the halo.