This galaxy exhibits an elliptical morphology, appearing primarily smooth in structure. It presents with an elongated profile, though not strongly cigar-shaped. The light distribution suggests a centrally concentrated bulge. There's evidence of possible disturbance, potentially indicative of minor gravitational interaction, though no major merger activity is immediately apparent. The galaxy displays a yellow-orange hue overall, hinting at an older stellar population with a suppressed rate of recent star formation. Based on apparent size and inferred distance, this is a relatively large galaxy in terms of physical extent. There are suggestions of tidal features, indicating a possible past or ongoing minor merger event.
