The galaxy presents an overall smooth, elliptical morphology. Its light distribution is centrally concentrated, with a bright, diffuse core that diminishes gradually towards the outer regions. The color profile appears relatively uniform, with a subtle reddish-yellow hue suggesting an older stellar population and/or significant dust obscuration. The galaxy’s shape appears elongated, exhibiting an approximate cigar-shaped morphology. There seems to be little evidence of prominent spiral arms, distinct dust lanes, or any obvious signs of ongoing major merger activity. Minor disturbances or tidal features may be subtly present, warranting further investigation with higher resolution imaging. The galaxy appears relatively isolated.
