The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a somewhat elongated, cigar shape in its overall form. The central region displays a concentrated, bright core, suggesting a higher density of stars in that area.  There's a gradual fading in luminosity as one moves outward from the core towards the edges of the galaxy, which appear indistinct and diffuse.  No distinct spiral arms or prominent dust lanes are discernible. There may be some minor disturbances or irregularities in the outer regions of the galaxy, but it does not appear to be actively undergoing a major merger. Overall, the galaxy appears to be dominated by an older stellar population.
