The galaxy presents as a relatively smooth, elliptical morphology, with a noticeable central bulge. The light is concentrated towards the center, exhibiting a yellowish hue, possibly indicative of an older stellar population. There is little evidence of spiral arm structures or active star formation regions. The galaxy appears to be moderately inclined relative to our line of sight, with a slightly elongated shape. The outer regions of the galaxy fade gradually into the background sky, suggesting a lack of distinct boundaries. Overall, the galaxy appears to be a mature system with a dominant spheroid component.
