The galaxy presents as a moderately bright, elliptical or lenticular structure, characterized by a smooth, centrally concentrated luminosity profile. The color is generally yellowish with a hint of redder hues in the outer regions, suggesting an older stellar population and moderate dust content. The object is elongated, exhibiting a minor-to-major axis ratio of approximately 0.8, with a slightly inclined disk or spheroidal shape. There are no obvious signs of spiral arms or significant star formation regions. The overall appearance indicates a relatively evolved galaxy with a small amount of ongoing star formation.
