The galaxy presents as a relatively smooth and concentrated object. Its shape appears to be somewhat elliptical, with the isophotes gradually fading away from the center. The core exhibits a bright, yellowish hue, suggesting an older stellar population and potentially a lack of significant ongoing star formation within the central regions. There is no discernible spiral structure or bar feature. There is little if any evidence of tidal disturbances or recent merger activity in this image. Overall, the galaxy seems to be a fairly quiescent system, consistent with an elliptical classification.
