The galaxy presents a morphology indicative of an elliptical galaxy, exhibiting a generally smooth and diffuse light distribution. The shape appears somewhere between round and elongated, with a slight cigar-like aspect ratio. Color gradients suggest a population of older stars that are more centrally concentrated, contributing to the overall redder hue observed towards the galactic core. There are no prominent dust lanes or spiral arm structures visible, consistent with a lack of significant ongoing star formation. The galaxy does not exhibit any obvious signs of a major merger or tidal disturbance.