The galaxy appears to be a relatively smooth, elliptical-type system. It exhibits a concentrated central bulge, characterized by a yellowish hue, possibly indicative of an older stellar population. Moving outward from the core, the light becomes slightly bluer, suggesting the presence of younger stars in the outer regions. The galaxy's overall shape is elongated, appearing somewhat cigar-shaped rather than perfectly spherical. There are no prominent spiral arms or dust lanes visible. Faint hints of asymmetry are present, possibly suggesting a minor interaction or disturbance event in its recent history.
