The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution without discernible spiral arms or a prominent disk structure. The central bulge is bright and concentrated, gradually fading into an extended halo. Color gradients suggest a population of older stars dominating the galaxy, particularly in the bulge region. The overall shape appears largely rounded, with a slight deviation towards a cigar-shaped structure. There is no immediate visual evidence of significant ongoing star formation, or tidal disturbances indicative of recent merger events. The galaxy shows no prominent dust lanes or patchy star forming regions.
