The galaxy appears to be a relatively smooth, elliptical system. It exhibits a slightly elongated morphology, trending toward an "in-between" roundness, not perfectly spherical, nor distinctly cigar-shaped. The central region displays a concentrated luminosity profile. There is some indication of minor disturbances, evidenced by subtle asymmetries in the light distribution, but the overall structure suggests it is not undergoing a major merger. The galaxy presents a color gradient, with the core tending toward redder hues and the outer regions trending toward blue. The estimated effective radius suggests a moderately sized system. The overall observed color suggests ongoing, but relatively low, star formation activity.
