The galaxy presents as a relatively smooth, elliptical structure. It appears to be quite concentrated, with a bright central bulge that dominates the overall light profile. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a slightly bluer hue in the outer regions. The shape appears somewhat elongated, potentially exhibiting a cigar shape. No distinct spiral arm structures or prominent dust lanes are discernible, suggestive of a relatively passive galaxy with a low star formation rate. There is a very small indication of some type of minor disturbance in the evenness of the galaxy, although this is difficult to assess.
