The galaxy exhibits a smooth, elliptical morphology with a high degree of central concentration. Its color profile is dominated by redder hues, indicative of an older stellar population, although hints of bluer colors are present in the outer regions. The overall shape is elongated, exhibiting a degree of flattening. No distinct spiral arms or prominent dust lanes are discernible, consistent with a relatively undisturbed, evolved system. The object appears to be a field galaxy, as there are no obvious signs of tidal interactions or nearby companions. The light distribution suggests a Sersic profile, implying the galaxy likely formed through mergers and accretion events.
