The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. Its overall shape appears approximately elliptical, exhibiting a radial color gradient. The core displays a yellowish-white hue, suggesting a population of older stars. The outer regions transition to a redder color, potentially indicating a lower rate of recent star formation or a higher abundance of dust attenuating blue wavelengths. There is no strong evidence of spiral arm structure or distinct dust lanes. Faint, subtle extensions may be present along the major axis, possibly indicative of tidal features or a weak disk component. The system shows no obvious signs of a recent major merger event, although the subtle extensions suggest a possible minor interaction in its past. The galaxy's relatively compact size and high central concentration suggest a relatively massive system.
