The galaxy presents a generally smooth, elliptical morphology, with a notable concentration of light towards the central region. The light distribution suggests a well-defined nucleus, gradually fading into the outer regions. The overall color profile appears relatively uniform, with a slight reddening towards the center, indicating a potentially older stellar population in that region. There is no clear evidence of prominent spiral arms or significant dust lanes. The shape appears moderately elliptical, though it is difficult to determine without more precise measurements. No signs of ongoing major merger events or tidal disturbances are apparent in this image. The galaxy appears to be relatively isolated, without any nearby companions that would indicate a strong interaction.
